In: Wagner W., Székely, B. (eds.): ISPRS ТС VII Symposium - 100 Years ISPRS, Vienna, Austria, July 5-7, 2010, IAPRS, Vol. XXXVIII, Part 7B
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PROSPECTIVE SPACE MISSIONS WITH L-BAND MICROWAVE
RADIOMETRIC SYSTEMS
Yu. Tishchenko 3 , V. Savorskiy 3 , M. Smirnov 3 , V. Ablyazov b , A. Khaldin b
a Fryazino Department, Kotelnikov Institute of Radioengineering and Electronics, RAS,
Vvedenskogo sq., 1, Fryazino, Moscow region, 141190, Russia - (savor, tishchen)@ire.rssi.ru
b Special Design Bureau of the Institute of Radioengineering and Electronics RAS,
Vvedenskogo sq., 1, Fryazino, Moscow region, 141190, Russia - ahaldin@sdb.ire.rssi.ru
Commission VII, Working Group VII/5
KEY WORDS: microwave radiometric systems, scientific programs, remote sensing, decimeter waves, small satellite, Russian
segment of International Space Station.
ABSTRACT:
Prospective Russian space missions include aims directed in developing and enhancing Earth remote sensing techniques by means of
microwave radiometry. New L-band (wavelength about 21 cm) microwave radiometric systems for space applications are
constructed in the Special Design Bureau of the Institute of Radioengineering and Electronics RAS. Scientific programs of
experiments with these instruments, which incorporate numerous proposals of Russian scientific organizations, are prepared in the
Institute of Radioengineering and Electronics RAS. The main goals of scientific programs are: development of radio physical Earth
remote sensing methods from space in L-band for investigation of physical events and processes in earth surface-atmosphere system;
investigation of external factors (galaxy emission, ionosphere, etc.) impact into measured parameters of investigated objects;
analysis of radio interference problems; development of new techniques for processing of data with different space resolution.
1. INTRODUCTION
Theoretical and experimental investigations show that L-band
radiometry is very prospective (optimal) for soil moisture and
sea surface salinity investigations. These measurements
practically not influenced by weather conditions in the
atmosphere. Now one of the most important problems for L-
band radiometry is the problem of radio interference (RFI). RFI
may be not so important in open ocean region, but are very
strong in urban areas. The second important problem consists in
necessity to make relatively large antenna for reasonable spatial
resolution of the instrument.
Despite this difficulties interest to investigations with use of
microwave radiometers in this band is very high. One of the
most powerful L-band instruments launched several months ago
is European project SMOS [1]. It contains very sofisticated
interferometric imaging radiometer MIRAS with synthetic
aperture antenna. In USA under developments is a project
SMAP with combination of microwave radiometer and
scatterometer [2]. In Russia under development are simpler
microwave radiometers for small satellite and for Russian
segment of International Space Station (ISS) [3]. Time of
SMOS and our instruments operation may overlap and it should
provide the possibility to compare some results.
2. SPACE L-BAND MICROWAVE RADIOMETRIC
SYSTEMS
Leading scientific organization for creation of payload for two
space projects with use of L-band radiometers is Kotelnikov
Institute of Radioengineering and Electronics of RAS (IRE
RAS). Head design organization of these radiometric systems is
Special Design Bureau of IRE RAS (SDB IRE RAS).
The first creating radiometric system PN1 consists of L-band
microwave radiometer with 2 beams antenna. It is compact
module and will be attached to the outer side of the small
satellite (planed launching - 2010). General specification of the
instrument is presented in the middle column of Table 1.
PN1
ALRS
Main frequency,
MHz
1410
1410
Bandwidth, MHz
20
20
Radiometric
sensitivity, K
0,2-0,3
0,2-0,3
Polarization
linear
linear
Number of beams
2
8
FOW, km
350
50
Swath width (at
orbit height 350
km), km
700
400
Power consumption,
VA
<60
120
Weight, kg
< 13
35
Size, mm
radiomete
400x300x50
r
800x510
1200x1920
antenna