Midcourse Space Experiment: Introduction to the Spacecraft, Instruments, and Scientific Objectives.

Mill, John D.; O'Neil, R. R.; Price, S. D.; Romicks, Gerald J.; Uy, O. Manuel; Gaposchkin, E. M.; Light, Glenn C.; Moore, W. W.; Murdock, T. L.; Stair, A. T.

doi:10.2514/3.55673

Cited by 177 publications

(66 citation statements)

References 4 publications

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“…During the period October 5-17, 1996, the MTM was operated at BLO in support of coordinated data collection events by the Midcourse Space Experiment (MSX) satellite [Mill et al, 1994]. Favorable conditions prevailed during the data collection window, yielding ten high-quality data sets (average length _=10 h).…”

Section: Observations and Analysesmentioning

confidence: 99%

Terdiurnal oscillations in OH Meinel rotational temperatures for fall conditions at northern mid‐latitude sites

Pendleton¹,

Taylor²,

Gardner³

2000

Geophysical Research Letters

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Section: Observations and Analysesmentioning

confidence: 99%

Terdiurnal oscillations in OH Meinel rotational temperatures for fall conditions at northern mid‐latitude sites

Pendleton¹,

Taylor²,

Gardner³

2000

Geophysical Research Letters

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“…The Ballistic Missile Defense Organization's (BMDO) Midcourse Space Experiment (MSX) satellite was launched into a near sun-synchronous 900km polar orbit on April 24, 1996. A general description of the spacecraft, instruments and scientific objectives is reported in Mill, et al (1994]). On MSX, of concern here, is the Ultraviolet and Visible Imagers and Spectrographic Imagers (UVISI) instrument.…”

Section: Introductionmentioning

confidence: 99%

Polar cap optical observations of topside (>900 km) molecular nitrogen ions

Romick¹,

Yee²,

Morgan³

et al. 1999

Geophysical Research Letters

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“…Cross matching between the MGPS survey and MIR data from the Midcourse Space Experiment (MSX; Mill et al 1994) has been used by Cohen & Green (2001) to identify H ii regions. However, MGPS images suffer from significant artefacts, a limited bandwidth (3 MHz), and poor spatial sensitivity that limits the ability to sample angular scales above ∼30 arcmin.…”

Section: Hindson Et Almentioning

confidence: 99%

A Large-Scale, Low-Frequency Murchison Widefield Array Survey of Galactic H ii Regions between 260 < l < 340

Hindson

Johnston‐Hollitt

Hurley‐Walker

et al. 2016

Publ. Astron. Soc. Aust.

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We have compiled a catalogue of H ii regions detected with the Murchison Widefield Array between 72 and 231 MHz. The multiple frequency bands provided by the Murchison Widefield Array allow us identify the characteristic spectrum generated by the thermal Bremsstrahlung process in H ii regions. We detect 306 H ii regions between 260° < l < 340° and report on the positions, sizes, peak, integrated flux density, and spectral indices of these H ii regions. By identifying the point at which H ii regions transition from the optically thin to thick regime, we derive the physical properties including the electron density, ionised gas mass, and ionising photon flux, towards 61 H ii regions. This catalogue of H ii regions represents the most extensive and uniform low frequency survey of H ii regions in the Galaxy to date.

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Midcourse Space Experiment: Introduction to the Spacecraft, Instruments, and Scientific Objectives.

Cited by 177 publications

References 4 publications

Terdiurnal oscillations in OH Meinel rotational temperatures for fall conditions at northern mid‐latitude sites

Terdiurnal oscillations in OH Meinel rotational temperatures for fall conditions at northern mid‐latitude sites

Polar cap optical observations of topside (>900 km) molecular nitrogen ions

A Large-Scale, Low-Frequency Murchison Widefield Array Survey of Galactic H ii Regions between 260 < l < 340

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