Abstract ======== This data set consists of the MESSENGER MASCS VIRS derived observations, also known as DDRs. The MASCS VIRS experiment is a fixed concave grating spectrograph with a beam splitter that simultaneously disperses the spectrum onto two photodiode arrays. There are two VIRS DDR data products, one for each array, which result in coverage of the wavelength ranges of the visible (VIS) and near infrared (NIR). This is version 2 of this data set; version 1 is available on PDS volume MESSMAS_2001.
Abstract ======== This data set consists of the MESSENGER MASCS VIRS derived observations, also known as DDRs. The MASCS VIRS experiment is a fixed concave grating spectrograph with a beam splitter that simultaneously disperses the spectrum onto two photodiode arrays. There are two VIRS DDR data products, one for each array, which result in coverage of the wavelength ranges of the visible (VIS) and near infrared (NIR). This is version 2 of this data set; version 1 is available on PDS volume MESSMAS_2001.
This dataset contains EDITED RAW DATA of the MARS Flyby (MSB). Included are the data of the very Flyby from February 23 until February 27,2007 and the data of the Passive Checkouts PC3 ( August 29, 2006), PC4 (November 23 - December 21,2006) and PC5 (May 22, 2007)
This dataset contains EDITED RAW DATA of the MARS Flyby (MSB).
Included are the data of the very Flyby from February 23 until
February 27,2007 and the data of the Passive Checkouts PC3
( August 29, 2006), PC4 (November 23 - December 21,2006) and
PC5 (May 22, 2007)
This dataset contains RAW DATA of the MARS Swingby Phase from 27 November 2006 until 24 February 2007. The closest approach (CA) took place on 25 February 2007
This dataset contains calibrated, 1.05- to 4.8-micron spectral images of comet C/Garradd (2009 P1) acquired by the High Resolution Infrared Spectrometer on 26 March and 02-03 April 2012 during the Cruise 3 phase of the EPOXI mission.
This dataset contains calibrated, 1.05- to 4.8-micron spectral images of comet C/Garradd (2009 P1) acquired by the High Resolution Infrared Spectrometer on 26 March and 02-03 April 2012 during the Cruise 3 phase of the EPOXI mission.
This dataset contains RAW DATA of the MARS Swingby Phase from 27 November 2006 until 24 February 2007. The closest approach (CA) took place on 25 February 2007