How to process radio occultation data: 1. From time series of frequency residuals to vertical profiles of atmospheric and ionospheric properties
Expertise in processing radio occultation observations, which provide vertical profiles of atmospheric and ionospheric properties from measurements of the frequency of radio signals, is not widespread amongst the planetary science community. In order to increase the population of radio occultation p...
Main Authors: | Withers, Paul, Moore, L., Cahoy, Kerri, Beerer, Ingrid Mary |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Aeronautics and Astronautics |
Format: | Article |
Language: | en_US |
Published: |
Elsevier
2016
|
Online Access: | http://hdl.handle.net/1721.1/105154 https://orcid.org/0000-0002-7791-5124 |
Similar Items
-
Physical characteristics and occurrence rates of meteoric plasma layers detected in the Martian ionosphere by the Mars Global Surveyor Radio Science Experiment
by: Withers, Paul, et al.
Published: (2017) -
Mars atmospheric CO2 condensation above the north and south poles as revealed by radio occultation, climate sounder, and laser ranging observations
by: Cahoy, Kerri, et al.
Published: (2017) -
Mars atmospheric CO[subscript 2] condensation above the north and south poles as revealed by radio occultation, climate sounder, and laser ranging observations
by: Hu, Renyu, et al.
Published: (2013) -
Analyzing Constellation Performance for the Radio Occultation Tomography of Internal Gravity Waves
by: Fitzgerald, Riley, et al.
Published: (2022) -
Direct imaging of exoEarths embedded in clumpy debris disks
by: Stark, C., et al.
Published: (2013)