Publications by authors named "Yingna Su"

Some geomagnetic storms' solar origins are ambiguous, making them hard to predict. On March 23, 2023, a severe geomagnetic storm occurred, however, forecasts based on remote-sensing observations failed to predict it. Here, we show clear evidence that this storm originates from the eruption of a trans-equatorial, longitudinal and low-density magnetic flux rope (FR) with weaker coronal emission and no chromospheric signs.

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In this paper, we propose a vanishing-point constrained Dijkstra road model for road detection in a stereo-vision paradigm. First, the stereo-camera is used to generate the u- and v-disparity maps of road image, from which the horizon can be extracted. With the horizon and ground region constraints, we can robustly locate the vanishing point of road region.

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Magnetic reconnection is a fundamental process of topology change and energy release, taking place in plasmas on the Sun, in space, in astrophysical objects and in the laboratory. However, observational evidence has been relatively rare and typically only partial. Here we present evidence of fast reconnection in a solar filament eruption using high-resolution H-alpha images from the New Vacuum Solar Telescope, supplemented by extreme ultraviolet observations.

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Article Synopsis
  • The Sun emits solar wind, a stream of ionized material, but its exact origin remains unclear.
  • Researchers used Hinode X-ray Telescope to observe a solar active region near a coronal hole, discovering a continuous outflow of soft X-ray-emitting plasmas.
  • These outflows are estimated to account for about 25% of the total mass loss rate of the solar wind, suggesting they could be a significant source of the solar wind itself.
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