![]() ![]() īlanco Rodríguez, J., Okunev, O.V., Puschmann, K.G., Kneer, F., Sánchez-Andrade Nuño, B.: On the properties of faculae at the poles of the Sun. Astronomical Society of the Pacific, San Francisco (2004)īerger, T.E., Rouppe van der Voort, L., Löfdahl, M.: Contrast analysis of solar faculae and magnetic bright points. (eds.) The Solar-B Mission and the Forefront of Solar Physics, Proceedings of the Fifth Solar-B Science Meeting, 12–14 November, 2003, Roppongi, Tokyo, Japan. In: 38th COSPAR Scientific Assembly, 18–15 July 2010, Bremen, Germany, p. 16 (2010)īerger, T.E., Title, A.M.: Recent progress in high-resolution observations. 175, 229–276 (2008)īarthol, P., Chares, B., Deutsch, W.: High resolution imaging and polarimetry with SUNRISE, a balloon-borne stratospheric solar observatory. 731(1), 29 (2011).Īvrett, E.H., Loeser, R.: Models of the solar chromosphere and transition region from sumer and HRTS observations: formation of the extreme-ultraviolet spectrum of hydrogen, carbon and oxygen. Īnđić, A., et al.: Response of granulation to small-scale bright features in the Quiet Sun. A model of a facular knot with the darkening core on the axis, which physically represents a micropore, stabilizing the entire magnetic configuration over a time interval of up to 1 day, is briefly described.Ībdusamatov, H.I., Krat, V.A.: Magnetic “knots” in the solar photosphere. A theoretical estimate of the characteristic scales of these structures in the photosphere is obtained as 20–30 km for the thickness of dark intergranular lanes (and the diameter of the thinnest magnetic tube in the solar photosphere), 200–400 km for the diameter of micropores. For intergranular lanes and micropores, a steady-state magnetic diffusion model is proposed, in which the horizontal-vertical plasma flows converging to a intergranular lane (and to the body of a micropore) compensate for the dissipative spreading of the magnetic flux at a given scale. The results due to image processing of micropores and facular knots obtained on modern adaptive optics telescopes are presented. As a separate constituent of the fine structure, a continuous net of dark intergranular lanes is considered. Photosphere google android#By introducing this feature, Google just ensured that there would be a street view image of every place possible, where an Android 4.2 device exists. +1 to you again, Google.Ĭan you think of some other fun daily-life uses of adding your Photosphere captures to Google Maps? I can think of a few naughty ones, but let’s hear your ideas first.The fundamental small-scale structures such as granules, faculae, micropores that are observed in the solar photosphere under high resolution are discussed. That’s really smart, Google – using the users to contribute to a service that they so often use. While StreetView already has a huge number of locations already available in its database, imagine the number of user-added images that are going to get added via this awesome feature. To add to that, the GPS location of the image is automatically tagged, and made available for others to view on Google Earth, Google+, and even Google Search. ![]() What’s even better, is that once you have clicked your PhotoSphere image, you can choose to upload it to Google Maps, which makes it available in its Street View app. Really awesome feature, which makes Panorama mode seem so passe. The PhotoSphere mode will allow you to capture 360° spherical views, or to be clearer, a 360° panoramic image, similar to the effect you get when you check out a Google Street View image. By now, we all know about the awesome PhotoSphere feature that the camera app in Android 4.2 is going to be equipped with. ![]()
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