Near-IR images of Comet 9P/Tempel 1 were obtained at the NASA IRTF during the period from June 24 through July 17, 2005 UT. These observations were taken as part of a campaign designed to support the science objectives of the Deep Impact spacecraft around the time of its encounter with Tempel 1. This data set contains all raw images, including those required for reduction and photometric calibration of the comet observations.

Near-IR spectra of Comet 9P/Tempel 1 were obtained with SpeX at the NASA IRTF during the period from June 24 through July 08, 2005 UT. These observations were taken as part of a campaign designed to support the science objectives of the Deep Impact spacecraft around the time of its encounter with Tempel 1 on July 4, 2005.

Near-IR spectra of Comet 9P/Tempel 1 were obtained with SpeX at the NASA IRTF during the period from June 24 through July 08, 2005 UT. These observations were taken as part of a campaign designed to support the science objectives of the Deep Impact spacecraft around the time of its encounter with Tempel 1 on July 4, 2005.

Mid-IR images of Comet 9P/Tempel 1 were obtained at the NASA IRTF during the period from July 2-18, 2005 UT. These observations were taken as part of a campaign designed to support the science objectives of the Deep Impact spacecraft around the time of its encounter with Tempel 1. This data set contains all raw images, including those required for reduction and photometric calibration of the comet observations.

IRTF Photometry of Io

The Cross-track Infrared Sounder (CrIS) Level 1B Full Spectral Resolution (FSR) data files contain radiance measurements along with ancillary spacecraft, instrument, and geolocation data of the CrIS instrument on the Joint Polar Satellite System-1 (JPSS-1) platform. This platform is also know as NOAA-20 (National Oceanic and Atmospheric Administration). The JPSS-1 mission with CrIS instrumentation is a follow-on to the Suomi National Polar-orbiting Partnership (SNPP) mission. The CrIS instrumentation and data processing system is nearly identical to that of the SNPP satellite. The FSR files have 2,223 channels (*2211 apodized channels): 637 (*633) shortwave channels from 3.9 to 4.7 microns (2555 to 2150 cm-1), 869 (*865) midwave channels from 5.7 to 8.05 microns (1752.5 to 1242.5 cm-1), and 717 (*713)longwave channels from 9.1 to 15.41 microns (1096.25 to 648.75 cm-1). Each CrIS field-of-regard (FOR) contains 9 field-of-views (FOVs) arranged in a 3X3 array. The Level 1B files contain 30 FORs in the cross track direction and 45 in the along track direction. Data products are constructed on six minute boundaries. The Visible Infrared Imaging Radiometer Suite (VIIRS) has 22 imaging and radiometric bands covering wavelengths from 0.41 to 12.5 microns. It provides the sensor data records for clouds, sea surface temperature, ocean color, and others. This IMG_COL product contains the colocation indices of the VIIRS pixels within each CrIS footprint.

이천에서 관측한 전리권 전자밀도 관측자료를 제공합니다. 해당 데이터가 보유한 컬럼은 다음과 같습니다. 컬럼명 : 관측시각, 위성번호, 신틸레이션 지수, TEC45, TEC30, TEC15, TEC0

This data set contains images of the Deep Space 1 target, comet 19P/Borrelly, and derived photometry from five consecutive nights of observing over 28 July - 1 August 2000. The observations were made using the 1.5m telescope of the Cerro Tololo Interamerican Observatory using the CFCCD camera mounted at the f/7.5 focus. The detector used was a Tek2K, yielding a plate scale of 0.4334 arcseconds/pixel. The photometric and lightcurve results were presented in Mueller and Samarasinha (2002).