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Robert C. Blanchard

Researcher at George Washington University

Publications -  65
Citations -  2248

Robert C. Blanchard is an academic researcher from George Washington University. The author has contributed to research in topics: Orbiter & Atmosphere. The author has an hindex of 21, co-authored 65 publications receiving 2141 citations. Previous affiliations of Robert C. Blanchard include Langley Research Center.

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Thermal structure of Jupiter's atmosphere near the edge of a 5‐μm hot spot in the north equatorial belt

TL;DR: This article measured the thermal structure of the atmosphere of Jupiter from 1029 km above to 133 km below the 1-bar level during entry and descent of the Galileo probe and confirmed the hot exosphere observed by Voyager (∼900 K at 1 nanobar).
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Measurements of thermal structure and thermal contrasts in the atmosphere of Venus and related dynamical observations: Results From the four Pioneer Venus Probes

TL;DR: The thermal structure of the Venus atmosphere and differences in structure with latitude (up to 60 deg) and clock hour (from midnight to 8 AM) have been measured in situ from a height of 126 km to the surface by instruments on the four Pioneer Venus entry probes as discussed by the authors.
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The structure of the upper atmosphere of mars: In situ accelerometer measurements from mars global surveyor

TL;DR: Throughout the MGS mission, thermospheric density bulges have been detected on opposite sides of the planet near 90 degreesE and 90 degreesW, in the vicinity of maximum terrain heights, suggesting a wave 2 pattern may be caused by topographically-forced planetary waves propagating up from the lower atmosphere.
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Mars Pathfinder Entry, Descent, and Landing Reconstruction

TL;DR: The Mars Path-Nder mission as mentioned in this paper demonstrated an innovative, low-cost, reliable method for placing a science payload on the surface of Mars and evaluated the spacecraft performance during entry, descent, and landing.
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Structure of the Atmosphere of Jupiter: Galileo Probe Measurements

TL;DR: Temperatures and pressures measured by the Galileo probe during parachute descent into Jupiter's atmosphere essentially followed the dry adiabat between 0.41 and 24 bars, consistent with the absence of a deep water cloud and with the low water content found by the mass spectrometer.