N
N. Rich
Researcher at United States Naval Research Laboratory
Publications - 26
Citations - 4220
N. Rich is an academic researcher from United States Naval Research Laboratory. The author has contributed to research in topics: Coronal mass ejection & Solar wind. The author has an hindex of 17, co-authored 24 publications receiving 3726 citations.
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Journal ArticleDOI
Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI)
Russell A. Howard,John D. Moses,Angelos Vourlidas,Jeffrey S. Newmark,Dennis G. Socker,Simon Plunkett,Clarence M. Korendyke,J. W. Cook,A. Hurley,Joseph M. Davila,William T. Thompson,O. C. St. Cyr,E. Mentzell,Kimberly I. Mehalick,James R. Lemen,Jean-Pierre Wuelser,Dexter W. Duncan,T. D. Tarbell,C. J. Wolfson,A. Moore,Richard A. Harrison,Nicholas R. Waltham,J. Lang,Christopher J. Davis,C. J. Eyles,H. Mapson-Menard,G. M. Simnett,Jean-Philippe Halain,Jean-Marc Defise,Emmanuel Mazy,Pierre Rochus,Raymond Mercier,Marie-Françoise Ravet,Franck Delmotte,F. Auchère,Jean-Pierre Delaboudiniere,Volker Bothmer,W. Deutsch,Dennis Wang,N. Rich,S. Cooper,V. Stephens,G. Maahs,R. Baugh,D. R. McMullin,T. Carter +45 more
TL;DR: The Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) is a five telescope package, which has been developed for the Solar Terrestrial Relation Observatory (STEREO) mission.
Journal ArticleDOI
A catalog of white light coronal mass ejections observed by the SOHO spacecraft
Seiji Yashiro,Seiji Yashiro,Nat Gopalswamy,G. Michalek,G. Michalek,G. Michalek,O. C. St. Cyr,O. C. St. Cyr,Simon Plunkett,N. Rich,Russell A. Howard +10 more
TL;DR: In this paper, the authors present a summary of the statistical properties of the CMEs, including the apparent central position angle, the angular width in the sky plane, and the height (heliocentric distance) as a function of time.
Journal ArticleDOI
The dynamical nature of coronal streamers
TL;DR: In this article, high-sensitivity imaging of the Sun's white-light corona from space has revealed a variety of unexpected small-scale phenomena, including plasma blobs that are ejected continually from the cusplike bases of streamers, fine raylike structures pervading the outer streamer belt, and inflows that occur mainly during high solar activity.
Journal ArticleDOI
Heliospheric Images of the Solar Wind at Earth
N. R. Sheeley,A. D. Herbst,A. D. Herbst,C. A. Palatchi,C. A. Palatchi,Y.-M. Wang,Russell A. Howard,John D. Moses,Angelos Vourlidas,Jeffrey S. Newmark,Dennis G. Socker,Simon Plunkett,Clarence M. Korendyke,L. F. Burlaga,Joseph M. Davila,William T. Thompson,O. C. St. Cyr,Richard A. Harrison,Christopher J. Davis,C. J. Eyles,C. J. Eyles,Jean-Philippe Halain,Dennis Wang,N. Rich,Karl Battams,E. Esfandiari,Guillermo Stenborg +26 more
TL;DR: In this article, the authors compared the heliospheric images with in situ plasma and magnetic field measurements obtained by near-Earth spacecraft, and found a near perfect association between the occurrence of these waves and the arrival of density enhancements at the leading edges of high-speed solar wind streams.
Journal ArticleDOI
The Wide-Field Imager for Solar Probe Plus (WISPR)
Angelos Vourlidas,Russell A. Howard,Simon Plunkett,Clarence M. Korendyke,A. Thernisien,Dennis Wang,N. Rich,M. T. Carter,Damien H. Chua,Dennis G. Socker,Mark G. Linton,Jeff S. Morrill,Sean Lynch,Adam Thurn,Peter Van Duyne,R. Hagood,Greg Clifford,Phares J. Grey,Marco Velli,P. C. Liewer,Jeffrey R. Hall,E. M. DeJong,Zoran Mikic,Pierre Rochus,Emmanuel Mazy,Volker Bothmer,Jens Rodmann +26 more
TL;DR: The Wide-field Imager for Solar PRobe Plus (WISPR) as mentioned in this paper is the only image-based camera onboard the Solar Probe Plus (SPP) mission scheduled for launch in 2018 and employs a 95∘ radial by 58∘ transverse field of view.