. unfiltered . GGM02C model . PC 1 . PC 2+3 . PC 2 . PC 3 . PC 4 . PC 5 . Sum of nine first PCs 2-10 . Difference between the initial signal and ten first PCs 1-10 . PC 1 . PC 2+3 . PC 2 . PC 3 . PC 4 . PC 5 . Sum of nine first PCs 2-10 . Difference between the initial signal and ten first PCs 1-10 . PC 1 . PC 2+3 . PC 2 . PC 3 . PC 4 . PC 5 . Sum of nine first PCs 2-10 . Difference between the initial signal and ten first PCs 1-10 .

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The potential of plasma By Lisa Tidwell Astronaut Franklin Chang-Diaz, Director of the Advanced Space Propulsion Laboratory, works on the VASIMR engine. jsc2003e49523 Photo by James Blair Scott Winter, from Safety, Reliability & Quality Assurance, makes adjustments on the VASIMR. jsc2003e49525 Photo by James Blair A T A GLANCE HOW THE V ASIMR ENGINE WORKS The VASIMR engine works through a set of three linked magnetic cells. ... This plasma is what drives the rocket engine. ...

... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

... core . ... 54 љ void forward ( const Vec3d *altAzPos, float *mag, const int num=1) const ; . 55 љ void forward ( const Vec3f *altAzPos, float *mag, const int num=1) const ; . ... 57 љ void forward ( const float *sinAlt, float *mag, const int num) const ; . ... 59 љ void forward ( const float *sinAlt, float *mag) const ; . ... 68 љ void backward ( const float *sinAlt, float *mag, const int num=1) const ; . ... 89 љ static float SUBHORIZONTAL_AIRMASS; . ... 168 љ // static const QString source( . ...

... One striking feature is a small source of almost pure H 2 line emission, which is located near one of the compact sources in Orion reported by O'Dell and collaborators (HST-18 = 203-504). ... H-H objects, Proplyds, Orion Bar, H 2 . ... We obtained a series of images across the bright rim of the Orion Bar near the peaks of mm-wave molecular line emission with NICMOS cameras 1-3 (NIC1, NIC2, NIC3) in several filters on 1998 February 18. ... The suggestion of an H-H object does not seem compelling. ...

Собственные движения 413 звезд из каталога LSPM. ... Bytes Format Units Label Explanations 1- 11 A11 --- LSPM Designation of star in LSPM (I/298) 13- 14 I2 hh RAh Right Ascension J2000 , at Epoch (hours) 16- 17 I2 mm RAm Right Ascension J2000 , at Epoch (minutes) 19- 25 F7.4 ss RAs Right Ascension J2000 , at Epoch (seconds) 27 A1 --- DE- Declination J2000 , at Epoch (sign) 28- 29 I2 deg DEd Declination J2000 , at Epoch (degrees) 31- 32 I2 arcmin DEm Declination J2000 , at ...

. Webcams . Networking . Weather . Power . System health . Measurements . Sky status at Sun Apr 10 00:24:00 2016 is Clear Sky status at Sun Apr 10 00:24:00 2016 is Clear . Copyright 2007 2013.