Minimize FormoSat-2

FormoSat-2 / ROCSat-2 (Republic of China Satellite-2)

ROCSat-2 is an NSPO (National Space Program Office) of Taiwan Earth imaging satellite with the objective to collect high-resolution panchromatic (2 m) and multispectral (8 m) imagery for a great variety of applications such as in land use, agriculture and forestry, environmental monitoring, natural disaster evaluation, and in support of research interests, in particular with the ISUAL instrument. Daily image coverage of Taiwan and the surrounding region is required.

Background: A contract was signed in May 1999 between NSPO and DASA/DSS (Dornier Satelliten Systeme GmbH) of Germany to build a high-resolution optical imaging satellite. However, the German government refused to give DASA/DSS an export licence for the S/C (the People's Republic of China was protesting the deal). The stalemate was resolved in Dec. 1999 when NSPO signed a new contract with MMS (now Astrium SAS of France). Quick approval of the export of ROCSat-2 was provided by the French government. The ROCSat program is part of a long-term effort in Taiwan to develop an autonomous space capability.

Note1: A public naming competition took place in Taiwan in 2004 with regard to the ROCSat satellite program. At the end of this contest, the ROCSat program was given the new name of FormoSat in December 2004. Hence, ROCSat-2 became FormoSat-2.

Note 2: In 2005, the National Space Program Office was renamed to “National Space Organization”, keeping the same acronym, NSPO.

FormoSat2_Auto19

Figure 1: Artist's view of the FormoSat-2 spacecraft in orbit (image credit: NSPO) 1)

Spacecraft:

The spacecraft bus has been built by EADS Astrium SAS (prime contractor) of Vélizy, France, based on the Leostar 500 XO family. There were also contributions from Taiwanese industry (including satellite computers, S-band antennas, and sun sensors). The S/C structure consists basically of a hexagonal body of 1.6 m side length (diameter), 2.4 m in height.

The satellite is three-axis stabilized. The upper deck of the platform carries the payload (RSI and ISUAL) and also part of AOCS (Attitude and Orbit Control Subsystem), namely the star sensors, gyroscopes and an IRU (Inertial Reference Unit). The lower deck carries the four reaction wheels and the autonomous propulsion module. The pointing accuracy is < 0.7 km (0.12º); the position knowledge is < 70 m (0.02º).

The fixed solar array uses GaAs cells and consists of two deployable flaps. The entire S/C architecture is designed in such a way as to provide a low roll inertia, a key factor for satellite agility and instrument line-of-sight stability. The S/C provides a body-pointing capability of ±45º in roll and pitch (45º pitch in 60 s, 10º roll in 25 s, 30º roll in 60 s, respectively). The spacecraft wet mass is about 760 kg including 81 kg of propellant (N2H4) mass. The design life is five years or better. 2) 3) 4) 5) 6)

FormoSat2_Auto18

Figure 2: Illustration of FormoSat-2 (image credit: NSPO)

FormoSat2_Auto17

Figure 3: Illustration of FormoSat-2 spacecraft during prelaunch activiies (image credit: NSPO)

FormoSat2_Auto16

Figure 4: Schematic bus design of ROCSat-2 (image credit: NSPO)

S/C mass, power

764 kg (including fuel), 693 W (EOL)

S/C propellant

81 kg, N2H4

S/C pointing accuracy, knowledge

0.12º, 0.02º

Position knowledge of imagery

9 m

S/C pointing agility

Roll 10º in 25 s and 30º in 45 s, pitch 45º in 60 s

RF communication S-band (TT&C function)
RF communication in X-band
X-band modulation, polarization
X-band link margin at 20º elevation angle
X-band station G/T at 20º elevation angle

Data rate: 4 kbit/s uplink, 1.6 Mbit/s downlink
Data rate: 120 Mbit/s in downlink
NRZ-L, RHCP/LHCP (selectable)
>6 dB for clear sky
>31.3 dB for clear sky

Onboard data storage capability

41 Gbit on SSR (Solid State Recorder)

Table 1: Overview of performance parameters of the ROCSat-2 spacecraft

FormoSat2_Auto15

Figure 5: Block diagram of the CDMU (Command and Data Management Unit), image credit: NSPO (Ref. 6)

Domestic components of FormoSat-2:

• OMU (Onboard Management Unit), developed by Acer Inc. OMU is the satellite's central control unit and the core of the secondary system for central commands and data processing. The objective of OMU is to control the satellite's operations, including the processing and execution of uploaded commands and the collection, processing, storage, and downloading the data of satellite's status. 7)

FormoSat2_Auto14

Figure 6: Illustration of OMU (image credit: NSPO)

• Onboard flight software module, developed by Tatung System Technologies Corp. The objective is to manage and control the satellite orbit, position, and operation. The flight software is responsible for the calculation of satellite position/orbit, operation of scientific instrument payload, and communication with ground antenna.

• Sun sensor, developed by Shihlin Electric & Engineering Corporation. The objective is to determine the spacecraft's relative position to the sun according to the direction of the source of sunbeam.

FormoSat2_Auto13

Figure 7: Illustration of the sun sensor (image credit: NSPO)

• S-band antennas, designed and manufactured by Victory Industrial Corp. These antennas are responsible for receiving commands and transmitting microwave signals. They allow the uploading and downloading of the ground commands and satellite information.

FormoSat2_Auto12

Figure 8: View of the S-band antennas (image credit: NSPO)

• Flight harness, designed and manufactured by Aerospace Industrial Development Corp. The harness wirings are used for connecting satellite components and payload and for transmitting power, commands, and signals.

• Vertical installation dolly, designed and manufactured by Taiwan Aerospace Corp. It is the main loading equipment for the satellite integration and testing procedures. It has anti-shock and anti-tilting functions and can prevent people from approaching too close to the dolly.

• Satellite primary structure, designed, analyzed and tested by NSPO and manufactured by Aerospace Industrial Development Corp. and Taiwan Aerospace Corp. The satellite primary structure carries the different satellite components and payloads.

FormoSat2_Auto11

Figure 9: Alternate view of the FormoSat-2 spacecraft (image credit: EADS Astrium)

 

Launch: A launch of ROCSat-2 took place on May 20, 2004 (UTC) on a Taurus-XL vehicle of OSC (Orbital Sciences Corporation) from VAFB, CA (maiden flight of Taurus-XL configuration which offers greater lift capability compared to previous versions of the Taurus rocket).

Orbit: Sun-synchronous circular orbit, mean altitude = 888 km, inclination = 99.1º, period of 102.9 minutes, the LTDN (Local Time of Descending Node) is 9:26 hours (14 orbits/day). The agility of the spacecraft provides a daily revisit capability for event/disaster monitoring.

Note: Following the early-orbit checkout, the initial satellite orbit has been raised from 728 km to 891 km altitude in the period May 23 to June 2, 2004. A total of 32 burns were performed by the propulsion module with 4 burns for inclination change, to enter into the mission orbit with an altitude of 891 km and an inclination of 99.14º.

 

FormoSat2_Auto10

Figure 10: Schematic for mission operations during various orbital phases (image credit: NSPO)

 


 

Mission status:

• 2014: The FormoSat-2 mission is operating nominally. On May 21, 2014, FormoSat-2 will have been on-orbit for 10 years, with continuous monitoring for Taiwan and the world (the design life of 5 years has been doubled). 8)

- The remaining on-board propellant is 27 kg, which is sufficient for orbit maintenance of another 10 years.

- FormoSat-2 is currently in a good state of health, as investigations of the trending data of each subsystem verified (including RSI, C&DH, TT&C, Power, Thermal, Propulsion, and AOCS). The spacecraft experienced malfunctions of one gyro and one reaction wheel.

• Fall 2013: The FormoSat-2 satellite has been operated on orbit for more than 9 years (design life of 5 years). The RSI instrument is operated in the daytime (sunlit period), while the ISUAL is active during the nighttime (eclipse period) of the orbit. 9)

To meet both mission objectives and to accomplish conflict-free planning and scheduling, the mission operations have been more complicated than traditional dedicated Earth remote sensing satellites. For instance, the usage of the satellite’s limited onboard resources, especially the SSR (Solid State Recorder) and the power status, needs to be fully cross-checked before a command load generation for either mission objective of payload.

- Malfunction of the IRU (Inertial Reference Unit) and noise of gyro A: The IRU contains 4 gyros, 2 processing units and 2 power supplies; its configuration is illustrated in Figure 11. Gyro input axes are arranged in a skewed redundant configuration such that any of three of four gyro axes provides a full set of three-axis data, i.e., the gyros works in a 3 among 4 cold redundancies for the inertial attitude estimation purpose. Two processing units and two power supplies (PSs) are also redundant, i.e., only one for each is used in operation. In summary, the IRU features four gyros in a tetrahedron configuration, with a full redundancy for power supply and electronics.

The IRU anomaly was first found on February 7, 2006, the time was not yet the completion of 2 years on orbit operation. The configuration of using PS2/CPU2 and gyro A/B/C has been operated smoothly for about seven months. Unfortunately, the 2nd IRU malfunction happened in September 2006. This anomaly led to the 2nd IRU reconfiguration with gyro A off. From that time, the IRU was configured to use PS2/CPU2 and gyro B/C/D. Thanks to the full redundant considerations and cross-strap design, the IRU could be used without degrading its functions and performances even undergone these two malfunctions.

FormoSat2_AutoF

Figure 11: IRU configuration (gyro 1/2/3/4 equals A/B/C/D), image credit: NSPO

- Malfunction of the RW (Reaction Wheel) interface (Figure 12): The design concept of the reaction wheels in FormoSat-2 is to use a cluster of four wheels in hot redundancy, in order to take advantage of the degree of freedom to avoid wheel rate zero-crossing. The RWA (Reaction Wheel Assembly) consists of one RW and a single channel WDE (Wheel Drive Electronics).

The RW malfunction occurred in November 2009, while FormoSat-2 has been operated for five and a half years, exceeding design life around 6 months. The project managed to find a solution for this problem.

FormoSat2_AutoE

Figure 12: Schematic view of the 4 RW interfaces (image credit: NSPO)

- For more than 9 years of fully engaged operations, the FormoSat-2 spacecraft has encountered many anomalies, including 43 AROs (Automatic Reconfiguration Orders) and lots of error events. Most of the anomalies were transient incidents and the satellite could be switched back to normal situation shortly without interrupting the routine operations. The only permanent failures were the IRU malfunction and gyro-A noise and interface malfunction between RW3 and TIF (Telecommand Interface) board. However, since the failure of IRU/gyro was replaced with spares, the handicapped three-wheel configuration with the degraded maneuver capability did cause significant impacts on the mission operations.

Except for the two permanent malfunctions and three-wheel induced operations impacts, the FormoSat-2 spacecraft behaved quite well. It is expected to be operated on orbit for the next decade under such an experienced mission operations team (Ref. 9).

• The FormoSat-2 spacecraft and its payload are operating nominally in the summer of 2012 - in its 9th year on orbit - providing imagery for the domestic needs of Taiwan as well as for the international community. Astrium GEO-Information Services is the sole distributor of the Formosat-2 satellite’s imagery outside of Taiwan.
The daily revisit capability of FormoSat-2 is due to its high agility (FOR of ±45º), its high resolution imagery and quick response; they are a great asset for the coverage of disaster events on a global scale. This service has been requested quite frequently by countries stricken by disasters. - The spacecraft is in good health and expected to make more contributions in its extended mission life. 10)

• On March 11, 2011, an earthquake of magnitude 9.0 struck Japan, and the resulting 10 m high tsunami swept the country’s northeast coast within 15 minutes. The United Nations Platform for Space-based Information for Disaster Management and Emergency Response started the International Charter on Space and Major Disasters to coordinate the satellites of different countries in acquiring images of disaster affected areas. 11) 12)

FormoSat2_AutoD

Figure 13: Quick look images of three strips of Sendai, Fukushima, and Ichihara on March 13, 2011 (image credit: NSPO)

FormoSat-2 responded rapidly to Japan's needs of information about the disaster-stricken regions. Once the first image of the affected area after the disaster was acquired and downloaded at noon on March 12, it was processed within 2 hours and published on GEMDAS (Global Environment Monitoring and Disaster Assessment System).

The role that GEMDAS played in the Japanese disaster can be attributed to three factors. The daily-revisit orbit and high agility of FormoSat-2, the automatic image processing system of the satellite (F2 AIPS), and the web-based geospatial information system used to make the images public all contributed to the effective disaster response (Ref. 11).

• The FormoSat-2 spacecraft and its payload are operating nominally in 2011. Although the mission is beyond its design life of 5 years, the health of the spacecraft is such that NSPO expects continued observations until the follow-on mission is launched.

Note: The FormoSat-2 mission is to be followed by the FormoSat-5 mission of NSPO with a launch scheduled for 2014. The PDR (Preliminary Design Review) of FormoSat-5 was completed on Dec. 16, 2010. 13)

FormoSat2_AutoC

Figure 14: FormoSat-2 satellite image showing in natural colors the Chuquicamata Copper Mine, Chile (image credit: NSPO, Astrium) 14)

• The spacecraft and its payload are operating nominally in the fall of 2010. The satellite successfully complements existing high spatial resolution imaging satellites such as SPOT-5, IKONOS, and QuickBird, among others, with its unique capability of daily revisits worldwide. FormoSat-2 has now been operated beyond its mission lifetime of five years and is in its extended mission phase. 15) 16) 17)

- Besides providing imagery for the domestic needs of Taiwan, the spacecraft is frequently being used to deliver high-resolution imagery for event monitoring applications. For the recent large disasters in the world, like southern Asia tsunami, Sichuan earthquake, typhoon Morakot over Taiwan, and Chile earthquake, FormoSat-2 took the first images almost every time, and provided the intensive monitoring images to domestic and international organizations for aftermath relief.

- Example of spacecraft agility: When the Sichuan earthquake occurred on May 12, 2008, FormoSat-2 was able to take imagery over the disaster area during its first pass; this was followed immediately by a +30º roll maneuver to dump the data to the NSPO ground station nearly 3000 km away in real-time. The agility of the spacecraft is in particular ideal for disaster monitoring support by shortening the data transfer time significantly.

- In the first five years of operation, ISUAL (Imager of Sprites and Upper Atmospheric Lightning) recorded more than 12,000 TLE events. Among them, ELVES (Emissions of Light and Very Low Frequency Perturbations from Electromagnetic Pulse Sources) are found to be the most abundant type (~80%) of TLEs (transient luminous events), whereas sprites and halos only combine to account for ~20%. The distribution of sprites and halos closely resemble that of the cloud-to-ground lightning. However, nearly 60% of ELVEs occurred over the ocean, a feature indicating that the high peak current lightning is more abundant over the ocean (Ref. 15).

• After 5 years of operations, the spacecraft is still in a generally very good state-of-health condition and is expected to provide its services for several years (3 to 5) to come. 18)

• In Feb. 2009, NSPO issued a RFP (Request for Proposal) for the FormoSat-5 Remote Sensing Instrument (RSI) to provide continuity of observation data. FormoSat-5 is planned for launch in 2013. 19)

• The spacecraft and its payload are operating nominally as of 2009. So far, the FormoSat-2 imagery has also been used in many applications on a global scale, such as disaster monitoring, land-use (change) detection and environmental monitoring.

• When the Sichuan Province of southwest China was hit by an earthquake of magnitude 7.9 on May 12, 2008, FormoSat-2 was among the first providing its imagery of the stricken region to the Chinese Academy of Sciences. 20)

• In the timeframe 2007/8, the high-resolution imagery of FormoSat-2 was being used by the government of Brazil to plan field interventions to stop illegal deforestation in progress in the Amazon basin. 21)

• In 2006, the IRU power supply failed and the behavior of gyro-A turned out to be rather noisy. Due to these events, the project was forced to use the redundant devices. Thanks to the full redundant design of the spacecraft operations could be continued (Ref. 15).

• In May 2006, NSPO implemented a F2T (FormoSat-2 Terminal) in Svalbard, Norway, to extend the data acquisition capability of the mission.

SOH (State-of-Health) trending during two years of mission operations (May 2004-May 2006) on five major subsystems, including AOCS and EPS (Electric Propulsion Subsystem), and one major payload have been conducted. All parameters were well within specifications. The C&DH and the TT&C do not exhibit any SOH problems so far. 22)

• In April 2005, NSPO implemented a terminal in Kiruna, Sweden, to serve as an additional receiving station.

• The high-resolution FormoSat-2 imagery was used extensively to monitor the devastation on the coasts of south-east Asia caused by the Tsunami that struck the Indian Ocean region on Dec. 26, 2004 (the epicenter of the undersea earthquake was off the coast of Sumatra, Indonesia - killing more than 225,000 people in 11 countries; in retrospect the earthquake was referred to as the “Great Sumatra-Andaman earthquake”). The imagery of FormoSat-2 proved extremely helpful to disaster relief activities and area reform tasks.
Following the Tsunami monitoring activities, imagery from FormoSat-2 has supported Hurricane Katrina relief in the Gulf of Mexico (August 2005), the October 2005 Pakistani earthquake recovery, and other natural disasters.

• Mission operations started in June 2004 (the checkout and performance verification for satellite bus and RSI were started on May 21 and completed through June 2004; all performance requirements of FormoSat-2 had been successfully verified in orbit). Besides providing imagery for the domestic needs of Taiwan, the S/C is frequently being used to deliver high-resolution imagery for event monitoring (coverage of the Tsunami in Asia on Dec. 26, 2004 and thereafter, coverage of Hurricane Katrina in Aug. 2005, coverage of Typhoons on the Pacific, coverage of earthquake regions, etc.). The spacecraft is operating nominally as of 2006. 23) 24) 25) 26)

FormoSat2_AutoB

Figure 15: Panchromatic image of Kao Hsiung, Taiwan observed in July 2004 (image credit: SPOT Image)

• NSPO has contracted to SPOT Image S. A. for the international distribution of FormoSat-2 images since June 2004.

• On 4 July 2004, ISUAL successfully observed the first images of sprites, sprite halo, and elves.

• It took 3 days to check the performance and function of all subsystems of satellite bus, and 11 days to raise the satellite from 723 km parking orbit to 888 km mission orbit. Then the primary payload, a remote sensing instrument (RSI), was turned on and the first image was taken on 4 June 2004 (Ref. 26).

 


 

Sensor complement: (RSI, ISUAL)

Generally, the RSI is operated during the daytime (requiring sun illumination) while the ISUAL instrument is active during the nighttime phase of the orbit. Without any payload activities during an orbit, the spacecraft is sun-pointing by default to maximize its energy. The spacecraft attitude during the eclipse phase is geocentric (nadir pointing) for RSI thermal regulation and for communication coverage purposes. The mode transition from sunlit to eclipse orbit takes place automatically. For RSI observations, the attitude pointing is geocentric by default.

 

RSI (Remote Sensing Instrument):

RSI is a pushbroom-type imager built by EADS Astrium SAS, France. RSI is made up of the camera and IPU (Instrument Processing Unit). The camera itself consists of the optical subassembly, the secondary structure, and the FPA (Focal Plane Assembly). The Korsch telescope (mirrors & structure) design and the focal plane structure are being made of SiC (Silicon Carbide). The video electronics, sequencer, DC/DC converter, and compression cards comprise the IPU. 27) 28) 29) 30)

Spectral bands:
1 PAN (Panchromatic band)
4 MS (Multispectral bands), nm


450-900 nm
B1= 450-520, blue
B2 = 520-600, green
B3 = 630-690, red
B4 = 760-900, NIR

Spatial resolution (GSD)

2 m for PAN, 8 m for MS imagery

Swath width

24 km

S/C body pointing capability, FOR (Field of Regard)

±45º in the roll and pitch axis ( providing a cross-track observation capability of 968 km about nadir for event/disaster monitoring); cross-track and along-track observation capability

Optics, focal length,
Aperture diameter

Cassegrain type optics with refractive corrector, focal length= 2896 mm, pupil diameter = 600 mm

Detector types

CCD: TH 7834 for PAN, THX 31547 quad-linear CCD for MS
Pan: 12,000 pixels, MS: 3,000 pixels

Integration time

0.308 ms for PAN, 1.232 ms for MS

Processing rate

10 Mpixel/s for PAN, 5 Mpixel/s for MS

Pixel quantization

12 bit

Data compression ratio

2.8 and 3.75 for PAN, 1.7 and 3.75 for MS

Instrument mass, power consumption

114 kg, 161 W for imaging, 73 W for standby

Table 2: Performance characteristics of RSI

RSI utilizes the agility of the satellite bus for stereo imaging over a specific region, continuous imaging over a slender region, and mosaic imaging over a large region. The imaging capability is 8 minutes per orbit, and the imaging areas during one cycle can be one 3000 km x 24 km continuous strip, two 100 km x 24 km stereo pairs, four 100 km x 24 km strips, or eight scenes.

FormoSat2_AutoA

Figure 16: Schematic structure of RSI (image credit: NSPO)

In-flight radiometric calibration: Although the RSI instrument was calibrated on-ground prior to launch with an uncertainty of 5%, the in-flight calibration has to be done regularly with the pre-flight calibration data as reference. The in-flight calibration includes two major parts: absolute and relative radiometric calibrations. Use of test sites in the ground segment. NSPO and CNES are using the following test sites: La Crau test site (43.56ºN, 4.86ºE) and desert sites Libya 1 (24.42ºN, 13.35ºE), Libya 2 (25.05ºN, 20.48ºE), Libya 3 (23.15ºN, 23.1ºE) and Mauritania 2 (20.85ºN, 8.78ºW), respectively. These sites are selected because of their spatial uniformity and temporal stability of the surface reflectance. 31) 32)

 

ISUAL (Imager of Sprites and Upper Atmospheric Lightning):

ISUAL is a joint international research program of NSPO, UCB (University of California at Berkeley), National Cheng Kung University of Taiwan, and Tohoku University, Japan. The objective is to observe the natural upward lightning discharge phenomena toward the ionosphere on top of the troposphere, referred to as TLEs (Transient Luminous Events). The requirements call for: 33) 34) 35)

• To determine the location and timing of luminous phenomena above thunder clouds to investigate their spatial, temporal and spectral properties

• To obtain a global survey of upper atmospheric optical flash transients (sprites, elves, blue jets, gigantic jets, etc.).

The instrument consists of four elements: a) intensified sprite imager, b) a six-channel spectrophotometer, c) a two-channel array photometer, and d) an electronics package. The imager is a staring-type frame CCD camera, taking 180 frames/s with a resolution of 512 x 80 pixels in a FOV of 20º x 3.15º. In Figure 18, the large disk of the ISUAL instrument contains six color filters, which can be rotated to select wavelength for measuring the emission spectrum of red sprites. ISUAL is operated in three modes:

• The sprite continuous mode to take images with a sample rate of 100 Hz

• The sprite burst mode with a sample rate of 1000 Hz

• The auroral mode at a constant rate of 1 sample/s.

All the instruments are mounted on a common platform and boresighted in the same direction. The imager is equipped with a six-filter wheel. ISUAL monitoring occurs during each nightside pass. The source data are stored and compressed in a separate 128 MByte memory. The data are downlinked in S-band. The total data volume is about 1 Gbit/day.

FormoSat2_Auto9

Figure 17: Functional block diagram of the ISUAL instrument (image credit: UCB/SSL)

The selection of filters are:

1) 623-750 nm - N2 1st positive band filter for observing sprites, removing the lightning induced at 777.4 nm line and minimizing the contribution of the airglow in the 760 nm O2 band

2) 762 nm - O2 (0,0) atmospheric band for observing airglows and auroras

3) 427.8 nm - energetic electron induced emissions of sprites and auroras

4) 630 nm - aurora and airglow emissions

5) 557.7 nm - aurora and airglow emissions

6) blank filter with IR blocking by the camera lens.

The photometers are fitted with the following filters:

1) 150-280 nm - bandpass ultraviolet filter to look at N2 LBH bands

2) 250-390 nm - bandpass ultraviolet filter; for sprites emission in this range with attenuating lightning contamination

3) 337.0 nm - N2 2nd positive narrow band filter to act as a particle energy spectrometer

4) 427.8 nm - narrow band filter to function as an energetic electron detector in sprites and aurora

5) 623-750 nm - bandpass filter to detect N2 1st positive emission from sprites

6) 777.4 nm - narrow band filter to detect lightning and act as a possible TLE event trigger.

The two array photometers are identical in every aspect, except one fitted with a blue band filter and another equipped with a red band filter. The wavelength selections for the two array photometers are 360-450 nm and 525-880 nm, respectively.

FormoSat2_Auto8

Figure 18: Illustration of the ISUAL instrument with sprite imager (left) and spectrophotometer at right (image credit: NSPO)

The imager is designed to capture five images in quick sequence. The imager operates continuously and five data frames are captured when the photometer signals the presence of a flash event in the field of view. This method of operation obtains high temporal resolution framing of the image.

FormoSat2_Auto7

Figure 19: Schematic view of the imager with filter wheel (image credit: UCB/SSL)

FormoSat2_Auto6

Figure 20: Imager optics of sensor layout (image credit: UCB/SSL)

FormoSat2_Auto5

Figure 21: Spectrophotometer sensor head (image credit: UCB/SSL)

FormoSat2_Auto4

Figure 22: TLEs generated by the upward discharge from thundercloud to the ionosphere (image credit: V. P. Pasko, 2007)

 

Status of ISUAL

• In 2014, FORMOSAT-2’s scientific payload ISUAL is still operational (Ref. 8).

• During the period July 4, 2004 to May 31, 2013, ISUAL recorded 31,369 TLEs (Transient Luminous Events); of this total sum, there were the following classes of TLEs according to their appearances: 73.65% elves, 6.53% red sprites, 6.00% halos, 13.51% blue jets, and 0.30% gigantic jets. 36)

Due to the orbital characteristics of FORMOSAT-2, unobserved gaps exist between each two orbits. Also, the ISUAL has its detection threshold. An estimated global occurrence rate is 24 TLEs per minute, but this number is still much less than the possible potential rate of 195.

Year

Elves

Sprites

Halos

Blue Jets

Gigantic Jets

Total

2004

588

68

67

37

0

760

2005

1420

217

165

124

7

1933

2006

2212

201

258

239

5

2915

2007

2653

255

277

398

6

3589

2008

2643

188

163

507

16

3517

2009

3046

261

218

510

16

4051

2010

3195

250

234

697

16

4392

2011

3394

300

258

718

14

4684

2012

3016

217

190

639

15

4077

2013

937

91

53

370

0

1451

Total (%)

23,104 (73.65)

2,048 (6.53)

1,883 (6.0)

4,239 (13.51)

95 (0.30)

31,369 (100)

Table 3: Number of TLEs observed by ISUAL from 4 July 2004 to 31 May 2013

Year

Aurora

TLE

Airglow

Total

Orbits

Hours

Orbits

Hours

Orbits

Hours

Orbits

Hours

2004

21

1.01

1225

406.09

19

6.77

1265

413.86

2005

24

1.12

3064

1050.95

34

5.45

3122

1057.52

2006

159

9.06

3821

1274.17

305

93.38

4285

1376.61

2007

217

11.99

4128

1424.16

405

136.13

4750

1572.28

2008

217

17.78

3823

1317.78

572

188.61

4612

1524.17

2009

102

5.76

4192

1402.64

272

175.09

4566

1583.49

2010

0

0.00

4054

1408.46

255

85.47

4309

1493.93

2011

0

0.00

4140

1454.55

0

0.00

4140

1354.55

2012

41

3.25

3479

1221.99

613

153.19

4133

1378.44

2013 (May 31)

0

0.00

1340

484.89

314

66.20

1654

551.09

Total

781

49.97

33,266

11445.69

2789

910.29

36836

12405.95

Table 4: Accumulated observation orbits and hours of ISUAL from 4 July 2004 to 31 May 2013

FormoSat2_Auto3

Figure 23: Global distribution of 31,369 TLEs observed by ISUAL from 4 July 2004 to 31 May 2013 (image credit: NSPO, Ref. 36)

FormoSat2_Auto2

Figure 24: The first Sprite image captured by ISUAL on July 4, 2004 over the Philippines (image credit: NSPO, Ref. 24)

 


 

Ground segment:

The basic elements of the ROCSat-2 ground segment are the SOCC (Spacecraft Operations and Control Center) and the XAS (X-band Acquisition System) located in Hsinchu, Taiwan. SOCC in turn consists of MOC (Mission Operations Center), MCC (Mission Control Center), SCC (Science Control Center), FDF (Flight Dynamics Facility), and GCN (Ground Communications Network). FormoSat-2 X-band imagery reception is also made available to third parties (international partners) with their own ground stations through cooperative agreements. 37) 38)

FormoSat2_Auto1

Figure 25: Major elements of the FormoSat-2 system architecture (image credit: NSPO, Ref. 5)

FormoSat2_Auto0

Figure 26: Architecture of the imaging processing system (image credit: NSPO)


1) http://www.nspo.org.tw/2008e/projects/project2/intro.htm

2) An-Ming Wu, Yung Liu, Lance Wu, Frank Wu, Ching-Jyh Shieh, “FormoSat-2 Satellite Images for Daily Monitoring,” Proceedings of the IAC 2005, Fukuoda, Japan, Oct. 17-21, 2005, IAC-05-B1.4.02

3) H. C. Wang, L. C. Lee, J. Ling, A. M. Wu, “ROCSat-2 Remote Sensing Mission,” Proceedings of the 51st IAF Congress, Rio de Janeiro, Brazil, Oct. 2-6, 2000, IAF-00-B.1.09

4) J. S. Chern, A. M. Wu, J. Ling, “Some Aspects of ROCSat-2 System Engineering,” Proceedings of the 3rd International Symposium of IAA, Berlin, April 2-6, 2001, pp. 57-60

5) Jeng-Shing Chern, An-Ming Wu, “Some aspects of ROCSAT-2 system engineering,” Acta Astronautica, Volume 54, Issue 2, January 2004, pp. 145-151

6) http://www.nspo.org.tw/2008e/projects/project2/property.htm

7) http://www.nspo.org.tw/2008e/projects/project2/component.htm

8) Information provided by Franz Ming-Chih Cheng, NSPO/NARLabs (National Applied Research Laboratories), HsinChu, Taiwan.

9) Shin-Fa Lin, Jeng-Shing Chern, An-Ming Wu, “Optimization on Mission Operations of the Handicapped FormoSat-2,” Proceedings of the 64th International Astronautical Congress (IAC 2013), Beijing, China, Sept. 23-27, 2013, paper: IAC-13-B4.3.5

10) An-Ming Wu, Guey-Shin Chang, Vicky Chu, “FormoSat-2 Daily Monitoring Around the World,” Proceedings of the 63rd IAC (International Astronautical Congress), Naples, Italy, Oct. 1-5, 2012, paper: IAC-12-B1.4.9

11) Cheng-Chien Liu, Nai-Yu Chen, “Responding to natural disasters with satellite imagery,” SPIE Newsroom, 2011, URL: http://spie.org/documents/Newsroom/Imported/003758/003758_10.pdf

12) “FORMOSAT-2 Quick Response to Japan Earthquake,” NSPO, URL: http://www.nspo.org.tw/Japan_Earthquake/en/Japan_Earthquake-0313.htm

13) “One more step forward for launching FORMOSAT-5,” URL: http://www.narl.org.tw/en/event/event.php?event_id=337

14) http://www.astrium-geo.com/na/1038-formosat-2

15) An-Ming Wu, Shin-Fa Lin, “Five Years Development and Five Years Operations of FORMOSAT-2 Satellite,” Proceedings of the 61st IAC (International Astronautical Congress), Prague, Czech Republic, Sept. 27-Oct. 1, 2010, IAC-10-D1.5.5

16) An-Ming Wu, Guey-Shin Chang, “Quick Response for Disaster Monitoring from FORMOSAT-2 Satellite,” Proceedings of the 61st IAC (International Astronautical Congress), Prague, Czech Republic, Sept. 27-Oct. 1, 2010, IAC-10-B1.1.6

17) Kun-Shan Chen, An-Ming Wu, Jeng-Shing Chern, Liang-Chien Chen, Wen-Yen Chang, “FormoSat-2 Mission: Current Status and Contributions to Earth Observations,” Proceedings of IEEE, May 2010, Vol. 98, Issue 5, pp. 878-891

18) Jeng-Shing Chern, An-Ming Wu, Shin-Fa Lin, “Post Mission Life Plan for FormoSat-2,” Proceedings of the 60th IAC (International Astronautical Congress), Daejeon, Korea, Oct. 12-16, 2009, IAC-09.B4.3.9

19) “Request for Proposal For the FORMOSAT-5 Remote Sensing Instrument (RSI) Opto-Mechanics Consultant Contract (RFP No. NSPO-RFP-0509),” NSPO, Feb. 11, 2009, URL: http://www.narl.org.tw/ext/po/po_attach.php?po_file_id=9483

20) Nancy Aktinson, “Satellite Images of China Earthquake,” Universe Today, May 16, 2008, URL: http://www.universetoday.com/2008/05/16/satellite-images-of-china-earthquake/

21) Florence Baillarin, Ghislain Gonzales, Carlos Souza, “Use of FormoSat-2 Satellite Imagery to Detect Near Real Time Deforestation in Amazonia,” Proceedings of IGARSS 2008 (IEEE International Geoscience & Remote Sensing Symposium), Boston, MA, USA, July 6-11, 2008

22) J.-S. Chern, A.-M. Wu, Shin-Fa Lin, “Two-Year State of Heat Trending of FormoSat-2,” Proceedings of the 57th IAC/IAF/IAA (International Astronautical Congress), Valencia, Spain, Oct. 2-6, 2006, IAC-06-B5.3.04

23) L. Wu, S.-S. Chen, J. Ju-Chen Yaung,, “Space Program in Taiwan,” Proceedings of ASC (Asian Space Conference), Chiang Mai, Thailand, Nov. 22-26, 2004

24) J.-S. Chern, “In Orbit Performance Verification of FormoSat-2,” Proceedings of the 5th IAA Symposium on Small Satellites for Earth Observation, Berlin, Germany, April 4-8, 2005

25) An-Ming Wu, Lance Wu, “Integrated Mission Planning for FormoSat-2 Imaging Satellite and FormoSat-3 Meteorological Constellation,” Proceedings of the 57th IAC/IAF/IAA (International Astronautical Congress), Valencia, Spain, Oct. 2-6, 2006, IAC-06-B1.6.09

26) J.-S. Chern, A.-M- Wu, S.-F. Lin, “Lesson learned from FORMOSAT-2 mission operations,” Acta Astronautica, Vol. 59, Issues 1-5, July-September 2006, pp. 344-350

27) A.-M. Wu, F. Wu, C.-J. Shieh, ”Daily Repetitive Imaging from ROCSat-2 Satellite,” Proceedings of IAC 2004, Vancouver, Canada, Oct. 4-8, 2004, IAC-04-IAF-B.5.06

28) http://www.nspo.org.tw/2008e/projects/project2/instrument.htm

29) Cheng-Chien Liu, “Processing of FORMOSAT-2 Daily Revisit Imagery for Site Surveillance,” IEEE Transactions on Geoscience and Remote Sensing, Vol. 44, No 11, Nov. 2006, pp. 3206-3214

30) Cheng-Chien Liu, “Processing of FORMOSAT-2 imagery for site surveillance,” Proceedings of 26th ACRS ((Asian Conference on Remote Sensing), Hanoi, Vietnam, Nov. 7-11, 2005

31) Kuo-Hsien Hsu, Shih-Chieh Chou, Li-Hsueh Chang , Nai-Yu Chen, “The In-flight Radiometric Calibration of FormoSat-2 Remote Sensing Instrument,” The Fourth Asian Space Conference 2008, Taipei, Taiwan, October 1-3, 2008

32) I. Benhadj, R. Hadria, B. Duchemin, V. Simonneaux, M. Le Page, B. Mougenot, O. Hagolle, G. Dedieu, “High Spatial and Temporal Resolution FormoSat-2 Images: First Results and Perspectives for Land Cover Mapping of Semiarid Areas (Marrakech/Al Haouz plain),” 2007, URL: http://trema.ucam.ac.ma/Irrimed/overview/morocco/Multitemp_2007_Benhadj_2.pdf

33) “The ROCSAT 2 ISUAL investigation,” URL: http://sprg.ssl.berkeley.edu/sprite/ago96/isual/ROCSAT.html

34) J. L. Chern, R. R. Hsu, H. T. Su, S. B. Mende, H. Fukunishi, Y. Takahashi, L .C. Lee, “Global Survey of Transient Luminous Events by ROCSat-2 Satellite,” Journal of Atmospheric and Solar-Terrestrial Physics, Vol. 65, 2003, pp. 647– 659, URL: http://sprite.phys.ncku.edu.tw/NewSprite/article/doc/Global_Survey_of_Upper_Atmospheric_Transi.pdf

35) http://sprite.phys.ncku.edu.tw/En/Eindex.html

36) Jeng-Shing Chern, An-Ming Wu, Shin-Fa Lin, “Globalization Extension of Transient Luminous Events from FORMOSAT-2 Observation,” Proceedings of the 64th International Astronautical Congress (IAC 2013), Beijing, China, Sept. 23-27, 2013, paper: IAC-13-B4.2.1

37) http://www.nspo.org.tw/2008e/projects/project2/ground.htm

38) Igor Lampin, “FormoSat-2, KOMPSAT-2, AstroTerra,” GroundSegment Coordination Body Workshop 2007, Frascati, Italy, June 19-20, 2007, URL: http://earth.esa.int/gscb/papers/22_Lampin.pdf


The information compiled and edited in this article was provided by Herbert J. Kramer from his documentation of: ”Observation of the Earth and Its Environment: Survey of Missions and Sensors” (Springer Verlag) as well as many other sources after the publication of the 4th edition in 2002. - Comments and corrections to this article are always welcome for further updates.

Minimize Featured Images