Научная статья на тему 'ВЫСОКОЭКОНОМИЧНАЯ СПУТНИКОВАЯ СИСТЕМА НАБЛЮДЕНИЯ'

ВЫСОКОЭКОНОМИЧНАЯ СПУТНИКОВАЯ СИСТЕМА НАБЛЮДЕНИЯ Текст научной статьи по специальности «Медицинские технологии»

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СПУТНИКОВАЯ СИСТЕМА НАБЛЮДЕНИЯ / СЪЕМКА ЗЕМЛИ / ОПЕРАТИВНОСТЬ / ПОКРЫТИЕ / ОБЗОР / ОРБИТА

Аннотация научной статьи по медицинским технологиям, автор научной работы — An-Ming Wu

В настоящее время съемка Земли со спутников в оптическом, ИК и радиодиапазонах находит очень широкое применение. В статье сначала рассмотрен одиночный ИСЗ, предназначенный для высокооперативного глобального наблюдения с высоким разрешением. Затем рассмотрен вариант спутниковой системы, обеспечивающей больший охват и более высокую оперативность. Входящие в ее состав ИСЗ могут принадлежать как одной, так и разным странам. Покрытие экваториальных областей может быть обеспечено несколькими ИСЗ. Для обзора полярных областей необходимы значительные зоны обзора. Ежесуточный обзор и глобальное покрытие может быть обеспечено доступным по цене количеством ИСЗ с определенной зоной обзора. Принимая во внимание проблемы эксплуатации и полярное покрытие, рекомендовано использовать спутниковую систему с повышенной оперативностью и большими зонами обзора. Возможно использование в спутниковой системе комбинации экваториальных и полярных орбит.

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Текст научной работы на тему «ВЫСОКОЭКОНОМИЧНАЯ СПУТНИКОВАЯ СИСТЕМА НАБЛЮДЕНИЯ»

Электронный журнал «Труды МАИ». Выпуск № 34

www.mai.ru/science/trudy/

A Cost-Effective Imaging Satellite Constellation

An-Ming Wu

Abstract

Imaging satellites utilize optical, infrared, or radar sensors to conduct the Earth observations, which are now extensively applied to our daily life. In the beginning we considered one-satellite mission, which is required to implement with high-resolution sensors, short revisit cycle, and global coverage. Now we considered mission conducted with multiple satellites, which may be operated by same or different countries, to increase the spatial coverage and to reduce the revisit cycle. Equatorial coverage can be achieved with multiple satellites, but the polar coverage can be done with a large field of regard. Daily revisit and global coverage can be both satisfied by selection of affordable number of satellites with certain field of regard. When taking into account operation complexity and polar coverage, it is recommended to use a constellation with shorter repeat cycle and large field of regard. One can also combine it with an equatorial orbit of 0-deg inclination or a polar orbit of 90-deg inclination.

Introduction

Solutions for daily revisit may have three categories: a GEO to continuously monitor for large events, a daily-repeat LEO to focally monitor for specific regions, and a constellation to intensively monitor for international cooperation. For international cooperation to develop satellites, there are various scenarios for the roles and responsibilities, including breakdown in systems, components, manpower, cost, schedule, and data distribution.

Imaging satellites utilize optical, infrared, or radar sensors to conduct the Earth observations, which are now extensively applied to our daily life. In the beginning we considered one-satellite mission, which is required to implement with high-resolution sensors, short revisit cycle, and global coverage. Now we considered mission conducted with multiple satellites, which may be operated by same or different countries, to increase the spatial coverage and to reduce the revisit cycle. An example is the RapidEye mission using five satellites to achieve daily revisit [1], and another example is GEOSS to integrate the existing and planning satellites and related systems worldwide for the seamless Earth observations [2].

FORMOSAT-2 is currently the only one satellite with daily revisit and global coverage, since it possesses features of daily repeat, high altitude, and large field of regard [3]. During its four year mission after launched in 2004, the satellite could take the first-time images and continuously monitoring for most events.

The capability of one satellite is nevertheless limited. In most cases of disasters, the area of interest is larger than the swath of a satellite, and the demand time is urgent and frequent more than that of one satellite can provide. Most existing satellites are designed with revisit cycles of 2 to 3 days. That means a constellation of 2 or 3 satellites can meet the requirement of daily revisit. But to cover the Poles, multiple satellites do not supercede single one, since all satellites are not passing over the Poles if one consider the Sun-synchronous orbits only.

Revisit and repeat

Revisit cycle can be realized in maximum or mean. The mean revisit cycle represents the expectation from users, while the maximum revisit cycle reflects the risk that a satellite fails to meet the expectation. It occurred one disaster per one month averagely. The lessons learned are mainly three: satellite capabilities always limited, satellite response always later, and satellite operations always complicated. The occurrence is stochastic, but the relief of disaster is mandatory. Therefore, It may be useful to consider the "regular and quick satellite

constellation" to have the mission schedule of satellites independent for each day and for each orbit.

Repeat orbit can simply the mission operations, imaging scheduling, and image processing, especially for those with shorter repeat cycles of 1, 2, or 3 days.

Table 1 lists the altitudes and the inclinations of Sun-synchronous orbits varying with the mean motion with increment of the mean motion of 1/12 rev/day. Those with shorter repeat cycles of 1, 2, or 3 days are marked with bold face. The mean revisit cycle varying with the altitude for Sun-synchronous orbits is shown in Figure 1, from which we can see minimum mean revisit cycles fall on some of the orbits with shorter repeat cycles.

Table 1 Repeat Sun-Synchronous Orbits

Mean Motion (rev/day) Altitude (km) Inclination (deg)

14.000 888. 99.001

14.083 860. 98.876

14.167 831. 98.754

14.250 803. 98.634

14.333 775. 98.516

14.417 747. 98.401

14.500 720. 98.288

14.583 693. 98.177

14.667 666. 98.068

14.750 639. 97.961

14.833 613. 97.856

14.917 587. 97.753

15.000 561. 97.653

15.083 535. 97.554

15.167 510. 97.456

15.250 485. 97.361

15.333 460. 97.267

15.417 435. 97.175

15.500 411. 97.085

15.583 386. 96.997

15.667 362. 96.909

15.750 338. 96.824

15.833 315. 96.740

15.917 291. 96.657

16.000 268. 96.576

Figure 1 Mean Revisit Cycles for Various Field of Regard

Coverage

Imaging satellites are most operated in Sun-synchronous orbits to keep the sunlight condition and simplify the satellite design. Poles attract increasingly concerns for the global warming effects. Originally the imaging satellites are not required to cover the Poles, but now the situation is different. Equatorial coverage can be achieved with multiple satellites, but the polar coverage can be done with a large field of regard.

Figure 2 shows the required field of regard to cover the Equator and the Poles for the constellation of 1, 2, or 3 satellites phasing in the true anomaly or the right ascension of ascending node. One satellite at 888 km altitude, the field of regard to cover the Poles is 53.6 deg, which is at the limit for side looking with distortion ratio as high as 4.9. This is still useful in urgent needs for imaging of large disaster area. Two satellites at 720 km altitude (corresponding to 14.5 rev/day mean motion) can reduce the field of regard to 42.4 deg to cover the Equator. Three satellites at 666 km altitude (corresponding to 14.5 rev/day mean motion)

can reduce the field of regard to 33.8 deg to cover the Equator. But to cover the Poles they still need large field of regard.

Altitude (km)

Figure 2 Field of Regard (FOR) to Cover Equator and Poles FORMOSAT-2 is at 888 km altitude, and has taken the first high-resolution satellite

image of the Amundsen-Scott South Pole Station with 46 deg field of regard, as shown in

Figure 3 and 4 [3,4]..

Figure 3

Figure 4 Limit Imaging of Amundsen-Scott South Pole Station (90 deg S), 2006.10.6

Daily revisit and global coverage

Constellation with same inclination and altitude can be phasing in the true anomaly or

the right ascension of ascending node according to the requirement of same local solar time or

same GMT time. Daily revisit and global coverage can be both satisfied by selection of

affordable number of satellites with certain field of regard. When taking into account operation

complexity and polar coverage, it is recommended to use a constellation with shorter repeat

cycle and large field of regard.

The coverage of 14 rev/day orbit with 53.6 deg FOR is shown in Figure 5. 90

45 0 -45

Figure 5 Coverage of 14 rev/day Orbit with 53.6 deg FOR The coverage of 14.5 rev/day orbit with 45 deg FOR is shown in Figure 6, from which

we can also see the overlapping area even possessing one-day revisit. As a minimum, one

satellite visits on one day, and another satellite for the other day. When considering

international coperation, each partner owns one satellite, and operates two satellites with

mutual benefit, which is the lowest cost subject to daily revisit and global coverage.

Figure 6 Coverage of 14.5 rev/day Orbit with 45 deg FOR If the equatorial or polar coverage is required, a combination of Sun-synchronous orbits

with an equatorial orbit of 0-deg inclination or a polar orbit of 90-deg inclination may be a

straightforward solution, respectively.

Conclusion

Equatorial coverage can be achieved with multiple satellites, but the polar coverage can be done with a large field of regard. Daily revisit and global coverage can be both satisfied by selection of affordable number of satellites with certain field of regard. When taking into account operation complexity and polar coverage, it is recommended to use a constellation with shorter repeat cycle and large field of regard. One can also combine it with an equatorial orbit of 0-deg inclination or a polar orbit of 90-deg inclination.

References

1. George Tyc, Keith Tuthman, Daniel Shulten, Manfred Krischke, Michael Oxfort, Paul Stephens, Alex Wicks, Tim Butlin, Martin Sweeting, " RapidEye - A Cost Effective satellite Constellation for Commercial Remote Sensing", IAC-03-IAA.11.1.06, 54th International Astronautical Congress, 29 September-3 October 2003, Bremen, Germany, 2003.

2. Thomas Adang, Charles Bryant, Linda Moodie, Gerald Dittberner, "Group on Earth Observations (GEO) - GEO-NETCast", IAC-06-B1.6.01, 57th International Astronautical Congress, 2-6 October 2006, Valencia, Spain, 2006.

3. Cheng-Chien Liu, Yueh-Cheng Chang, Stefani Huang, Frank Wu, An-Ming Wu, Soushi Kato, Yasushi Yamaguchi, "First Space-Borne High-Spatial-Resolution Optical Imagery of the Antarctic from FORMOSAT-2", Antarctic Science, 2008.

4. An-Ming Wu, Frank Wu, Ching-Jyh Shieh, "Urgent Image Processing for a Daily Revisit Satellite", IAC-07-B1.4.07, 58th International Astronautical Congress, 24-29 September 2007, Hyderabad India, 2007.

Author

An-Ming Wu

National Space Organization, 8F, 9 Prosperity 1st Road, Science Park, Hsinchu, Taiwan Contacts: amwu@nspo.org.tw

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