Close up on a solar prominence, with startling clarity, the New Moon's disk slides between the new Solar Dynamics Observatory in geosynchronous orbit and it's constant view of the Sun. The inconstant Moon is our humbling reminder how comparatively little things often obscure our view of a much bigger picture [NASA/GSFC/SDO].
Sun and Moon - A first for the Solar Dynamics Observatory (SDO), and it was visually engaging too. On October 7, 2010, SDO observed its first lunar transit when the new Moon passed directly between the spacecraft (in its geosynchronous orbit) and the Sun. With SDO watching the Sun in a wavelength of extreme ultraviolet light, the dark Moon created a partial eclipse of the Sun.
These images, while unusual and cool to see, have practical value to the SDO science team. Karel Schrijver of Lockheed-Martin's Solar and Astrophysics Lab explains: "The very sharp edge of the lunar limb allows us to measure the in-orbit characteristics of the telescope e.g., light diffraction on optics and filter support grids. Once these are characterized, we can use that information to correct our data for instrumental effects and sharpen up the images to even more detail."
The image below shows a full disk version, view the larger story here.
These images, while unusual and cool to see, have practical value to the SDO science team. Karel Schrijver of Lockheed-Martin's Solar and Astrophysics Lab explains: "The very sharp edge of the lunar limb allows us to measure the in-orbit characteristics of the telescope e.g., light diffraction on optics and filter support grids. Once these are characterized, we can use that information to correct our data for instrumental effects and sharpen up the images to even more detail."
The image below shows a full disk version, view the larger story here.
No comments:
Post a Comment