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  1. No Access

    Article

    Geometric Localization of CMEs in 3D Space Using STEREO Beacon Data: First Results

    The geometric localization technique (Pizzo and Biesecker, Geophys. Res. Lett. 31, 21802, 2004) can readily be used with Solar Terrestrial Relations Observatory (STEREO) Space Weather Beac...

    Curt A. de Koning, V. J. Pizzo, D. A. Biesecker in Solar Physics (2009)

  2. Article

    Open Access

    Theoretical modeling for the stereo mission

    We summarize the theory and modeling efforts for the STEREO mission, which will be used to interpret the data of both the remote-sensing (SECCHI, SWAVES) and in-situ instruments (IMPACT, PLASTIC). The modeling...

    Markus J. Aschwanden, L. F. Burlaga, M. L. Kaiser, C. K. Ng… in Space Science Reviews (2008)

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  3. No Access

    Chapter

    Theoretical Modeling for the STEREO Mission

    We summarize the theory and modeling efforts for the STEREO mission, which will be used to interpret the data of both the remote-sensing (SECCHI, SWAVES) and in-situ instruments (IMPACT, PLASTIC). The modeling...

    Markus J. Aschwanden, L. F. Burlaga, M. L. Kaiser, C. K. Ng… in The STEREO Mission (2008)

  4. No Access

    Article

    The NOAA Goes-12 Solar X-Ray Imager (SXI) 2. Performance

    The Solar X-ray Imager (SXI) was launched on 23 July 2001 on NOAA’s GOES-12 satellite and completed post-launch testing on 20 December 2001. It was brought into operations on 21 January 2003. This paper docume...

    V. J. Pizzo, S. M. Hill, C. C. Balch, D. A. Biesecker, P. Bornmann… in Solar Physics (2005)

  5. No Access

    Article

    The NOAA Goes-12 Solar X-Ray Imager (SXI) 1. Instrument, Operations, and Data

    The Solar X-ray Imager (SXI) was launched 23 July 2001 on NOAA’s GOES-12 satellite and completed post-launch testing 20 December 2001. Beginning 22 January 2003 it has provided nearly uninterrupted, full-disk,...

    S. M. Hill, V. J. Pizzo, C. C. Balch, D. A. Biesecker, P. Bornmann… in Solar Physics (2005)

  6. No Access

    Article

    Corotating Interaction Regions in the Outer Heliosphere

    We discuss the structure and evolution of CIRs and their successors in the outer heliosphere. These structures undergo significant evolution as they are convected to greater heliocentric distances. A progressi...

    P.R. Gazis, F.B. McDonald, R.A. Burger, S. Chalov, R.B. Decker… in Space Science Reviews (1999)

  7. No Access

    Article

    Formation and Evolution of Corotating Interaction Regions and their Three Dimensional Structure

    Corotating interaction regions are a consequence of spatial variability in the coronal expansion and solar rotation, which cause solar wind flows of different speeds to become radially aligned. Compressive int...

    J.T. Gosling, V.J. Pizzo in Space Science Reviews (1999)

  8. No Access

    Chapter and Conference Paper

    Formation and Evolution of Corotating Interaction Regions and Their Three Dimensional Structure

    Corotating interaction regions are a consequence of spatial variability in the coronal expansion and solar rotation, which cause solar wind flows of different speeds to become radially aligned. Compressive int...

    J. T. Gosling, V. J. Pizzo in Corotating Interaction Regions (1999)

  9. No Access

    Chapter and Conference Paper

    Corotating Interaction Regions in the Outer Heliosphere

    We discuss the structure and evolution of CIRs and their successors in the outer heliosphere. These structures undergo significant evolution as they are convected to greater heliocentric distances. A progressi...

    P. R. Gazis, F. B. McDonald, R. A. Burger, S. Chalov… in Corotating Interaction Regions (1999)

  10. No Access

    Article

    Solar wind corotating stream interaction regions out of the ecliptic plane: Ulysses

    Ulysses plasma observations reveal that the forward shocks that commonly bound the leading edges of corotating interaction regions (CIRs) beyond ∼2 AU from the Sun at low heliographic latitudes nearly disappea...

    J. T. Gosling, S. J. Bame, D. J. McComas, J. L. Phillips… in Space Science Reviews (1995)

  11. No Access

    Chapter and Conference Paper

    Solar Wind Corotating Stream Interaction Regions Out of the Ecliptic Plane: Ulysses

    Ulysses plasma observations reveal that the forward shocks that commonly bound the leading edges of corotating interaction regions (CIRs) beyond ~2 AU from the Sun at low heliographic latitudes nearly disappea...

    J. T. Gosling, S. J. Bame, D. J. McComas, J. L. Phillips… in The High Latitude Heliosphere (1995)

  12. No Access

    Chapter and Conference Paper

    Flux Tube Shredding and Its Infrared Signature

    The interchange instability of solar magnetic flux tubes and possible stabilization mechanisms are reviewed. Special attention is paid to the influence of magnetic tension forces and the internal atmosphere, b...

    M. Bünte, O. Steiner, S. K. Solanki, V. J. Pizzo in Infrared Solar Physics (1994)