D M Hassler
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Explore the profile of D M Hassler including associated specialties, affiliations and a list of published articles.
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11
Citations
210
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Recent Articles
1.
Zeitlin C, Castro A, Beard K, Abdelmelek M, Hayes B, Johnson A, et al.
Life Sci Space Res (Amst)
. 2023 Nov;
39:76-85.
PMID: 37945092
We report the results of the first six years of measurements of so-called fast neutrons on the International Space Station (ISS) with the Radiation Assessment Detector (ISS-RAD), spanning the period...
2.
Zeitlin C, Hassler D, Ehresmann B, Rafkin S, Guo J, Wimmer-Schweingruber R, et al.
Life Sci Space Res (Amst)
. 2019 Aug;
22:89-97.
PMID: 31421853
We report the first long-term measurements of the radiation quality factor of energetic charged particles on the surface of Mars. The Radiation Assessment Detector (RAD) aboard the Mars Science Laboratory...
3.
Kohler J, Ehresmann B, Zeitlin C, Wimmer-Schweingruber R, Hassler D, Reitz G, et al.
Life Sci Space Res (Amst)
. 2015 Jul;
5:6-12.
PMID: 26177845
The Mars Science Laboratory spacecraft, containing the Curiosity rover, was launched to Mars on 26 November 2011. Although designed for measuring the radiation on the surface of Mars, the Radiation...
4.
Farley K, Malespin C, Mahaffy P, Grotzinger J, Vasconcelos P, Milliken R, et al.
Science
. 2013 Dec;
343(6169):1247166.
PMID: 24324273
We determined radiogenic and cosmogenic noble gases in a mudstone on the floor of Gale Crater. A K-Ar age of 4.21 ± 0.35 billion years represents a mixture of detrital...
5.
Zeitlin C, Hassler D, Cucinotta F, Ehresmann B, Wimmer-Schweingruber R, Brinza D, et al.
Science
. 2013 Jun;
340(6136):1080-4.
PMID: 23723233
The Mars Science Laboratory spacecraft, containing the Curiosity rover, was launched to Mars on 26 November 2011, and for most of the 253-day, 560-million-kilometer cruise to Mars, the Radiation Assessment...
6.
Hassler D, Rottman G, Lawrence G
Appl Opt
. 2010 Aug;
30(25):3575-81.
PMID: 20706428
Microchannel plate detectors are widely used for ultraviolet (UV) and extreme-ultraviolet (EUV) observations. Curved-channel microchannel plates, or C plates, provide an electron gain of approximately 10(6) in a single plate...
7.
Elmore D, Card G, Chambellan C, Hassler D, Hull H, Lecinski A, et al.
Appl Opt
. 2008 Feb;
37(19):4270-6.
PMID: 18285875
The scientific motivation, design criteria, and specifications for a new ground-based instrument to observe the Sun in the He i 1083-nm spectral line is described. The instrument employs a liquid-crystal...
8.
Comparison of the imaging characteristics of curved-channel and straight-channel microchannel plates
Osterman S, Rottman G, Hassler D, McClintock W, Lawrence G
Appl Opt
. 1997 Feb;
36(4):753-9.
PMID: 18250734
We have measured and compared the spatial fidelity of two types of microchannel plates over roughly half of their active area. Measurements of the spatial fidelity of curved-channel microchannel plates...
9.
Hassler D, Lemaire P, Longval Y
Appl Opt
. 1997 Jan;
36(1):353-9.
PMID: 18250681
The Solar Ultraviolet Measurements of Emitted Radiation (SUMER) instrument on the Solar and Heliospheric Observatory (SOHO) satellite is sensitive to the state of linear polarization of the incident radiation primarily...
10.
KOPP G, Derks M, Elmore D, Hassler D, Woods J, Streete J, et al.
Appl Opt
. 1997 Jan;
36(1):291-6.
PMID: 18250672
A Lyot-Ohman filter for imaging near the solar He i 1083-nm line is described. Fast and continuous spectral tunability is provided by nematic liquid crystals. This solid-state filter has a...