Heliospheric Images of the Solar Wind at Earth

By N. R. Sheeley, A. Herbst, C. Palatchi, Y. Wang, R. Howard, J. Moses, A. Vourlidas, J. Newmark, D. Socker, S. Plunkett and 14 more. 2008

138 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/8fc6ae4e22c50551f8559158cdc12852c567a458

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. N. Lugaz
2. A. Thernisien
3. A. Vourlidas
4. J. Davies
5. M. Temmer
6. T. Howard
7. R. Howard
8. Jan Luhmann

Citations in the corpus

• GEOMETRIC TRIANGULATION OF IMAGING OBSERVATIONS TO TRACK CORONAL MASS EJECTIONS CONTINUOUSLY OUT TO 1 AU (2010, methodology): “This new method enables geometric triangulation for HI1 and HI2 data, relaxes various assumptions needed in a model fit (e.g., Sheeley et al. 1999, 2008; Rouillard et al. 2008; Davies et al. 2009), and can accurately determine CME kinematics (both propagation direction and radial distance)…”
• Interplanetary Coronal Mass Ejections Observed in the Heliosphere: 1. Review of Theory (2009, background): “Recent observations by the STEREO spacecraft, especially those by the Heliospheric Imager instruments (e.g., Harrison et al. 2008; Sheeley et al. 2008; Webb et al. 2009) have inspired a new wave of interest in the dynamics of the interplanetary medium within the space physics community.”
• ON SUN-TO-EARTH PROPAGATION OF CORONAL MASS EJECTIONS (2013, methodology): “Figure 2 displays two synoptic views of the CME (left) from STEREO A and B and the time-elongation maps (right) produced by stacking the running-difference images within a slit along the ecliptic (e.g., Sheeley et al. 2008; Davies et al. 2009; Liu et al. 2010a).”
• RECONSTRUCTING CORONAL MASS EJECTIONS WITH COORDINATED IMAGING AND IN SITU OBSERVATIONS: GLOBAL STRUCTURE, KINEMATICS, AND IMPLICATIONS FOR SPACE WEATHER FORECASTING (2010, methodology): “A correlation study of solar wind stream interaction regions between HI2 images and in situ measurements at 1 AU seems to suggest a density threshold of about 15 cm−3 at 1 AU for HI2 observations (Sheeley et al. 2008).”
• The Wide-Field Imager for Solar Probe Plus (WISPR) (2014, background): “To study the details of these small-scale transients, we need high-resolution observations, as these transients commonly take up only a few pixels in current LASCO and SECCHI coronagraph observations (Sheeley et al. 2008; Rouillard et al. 2008, 2009).”