The Energetic Particles: Acceleration, Composition, and Transport (EPACT) investigation on the WIND spacecraft
- Published:
- Volume 71, pages 155–206, (1995)
- Cite this article
Abstract
The Energetic Particles: Acceleration, Composition, and Transport (EPACT) investigation is designed to make comprehensive observations of solar, interplanetary, and galactic particles over wide ranges of charge, mass, energy, and intensity using a combination of 8 different particle telescopes. This paper summarizes the scientific goals of EPACT and provides a detailed description of the instrument design and capabilities.
Electrons are measured from 0.2 to 10 MeV, primarily providing time markers for injections of solar particles. Hydrogen is measured from 1.4 to 120 MeV, and Helium is measured from 0.04 to 500 MeV nucl−1. The collection powers and energy ranges for heavier nuclei up to iron are ideal for observations of quiet-time populations such as particles accelerated by interplanetary shocks and the anomalous cosmic rays (thought to be accelerated at the boundary of the heliosphere). The large collection power available is also ideal for observations of3He,4He, and heavier nuclei in impulsive3He-rich solar events. There is even the possibility of observing ultra heavy nuclei (Z>30) in large solar events for the first time. Finally, there is a telescope designed to measure isotopes from He (3.4–55 MeV nucl−1) to Fe (12–230 MeV nucl−1), which is intended for solar particles, the anomalous cosmic rays and galactic cosmic rays. The overall capabilities of EPACT provide scientifically interesting measurements over all phases of the solar cycle. There will also be important opportunities for combined studies with other spacecraft, such as SAMPEX, Ulysses, and Voyagers 1 and 2.
This is a preview of subscription content, to check access.
Access this article
Subscribe and save
- Starting from 10 chapters or articles per month
- Access and download chapters and articles from more than 300k books and 2,500 journals
- Cancel anytime
Buy Now
Price excludes VAT (USA)
Tax calculation will be finalised during checkout.
Instant access to the full article PDF.
Similar content being viewed by others
The High-Energy Ion Telescope (HIT) for the Interstellar Mapping And Acceleration Probe (IMAP) Mission
Recent Developments in Particle Acceleration at Shocks: Theory and Observations
A Novel Explanation for the Arrangement of the Universe–Solar System–Planets–Earth. Part 3
Explore related subjects
Discover the latest articles, books and news in related subjects, suggested using machine learning.References
Barbier, L. M., Reames, D. V., and von Rosenvinge, T. T.: 1993,Proc. XXIII Int. Cosmic Ray Conf., Calgary 3, 222.
Miller, J. A. and Viñas, A. F.: 1993,Astrophys. J. 412, 386.
Perkins, M. A., Kristoff, J. J., Mason, G. M., and Sullivan, J. D.: 1969,Nucl. Inst. Methods 68, 149.
Reames, D. V.: 1990,Astrophys. J. Suppl. 73, 235.
Reames, D. V., Meyer, J. P., and von Rosenvinge, T. T.: 1994,Astrophys. J. Suppl. 90, 649.
Reames, D. V., Richardson, I. G., and Barbier, L. M.: 1991,Astrophys. J. Letters 382, L43
Simpson, J. A. and Garcia-Munoz, M.: 1988,Space Sci. Rev. 46, 205.
Temerin, M. and Roth, I.: 1992,Astrophys. J. 391, L105.
UTMC: 1990a, ‘UT1750AR RISC Microprocessor’, United Technologies Microelectronics Center (UTMC), Colorado Springs, Colorado, Data Sheet.
UTMC: 1990b, ‘UTD-R Gate Array Family’, United Technologies Microelectronics Center (UTMC), Colorado Springs, Colorado, Data Sheet.
von Rosenvinge, T. T., Barbier, L. M., and Reames, D. V.: 1993,Proc. XXIII Int. Cosmic Ray Conf., Calgary 3, 400.
Winkert, G.: 1992, IEEE Trans. on Nuc. Sci. 39, 789.
Rights and permissions
About this article
Cite this article
Von Rosenvinge, T.T., Barbier, L.M., Karsch, J. et al. The Energetic Particles: Acceleration, Composition, and Transport (EPACT) investigation on the WIND spacecraft. Space Sci Rev 71, 155–206 (1995). https://doi.org/10.1007/BF00751329
Received:
Issue date:
DOI: https://doi.org/10.1007/BF00751329
Share this article
Anyone you share the following link with will be able to read this content:
Sorry, a shareable link is not currently available for this article.
Provided by the Springer Nature SharedIt content-sharing initiative
