सनस्पॉट हिंदी उपयोग और उदाहरण

सौर अधिकतम और सौर न्यूनतम अधिकतम और न्यूनतम सनस्पॉट मायने रखता है।

""अविश्वसनीय: यात्रा के दौरान ड्रॉप-आउट आम हैं, खराब मौसम और सनस्पॉट गतिविधि के दौरान।

17 वीं शताब्दी के प्रारंभ से सनस्पॉट देखे गए हैं और सनस्पॉट समय श्रृंखला किसी भी प्राकृतिक घटना की सबसे लंबी, लगातार देखी गई (रिकॉर्ड की गई) समय श्रृंखला है।

सौर अधिकतम के दौरान, बड़ी संख्या में सनस्पॉट दिखाई देते हैं, और सौर विकिरण का उत्पादन लगभग 0.07% बढ़ता है।

सनस्पॉट्स में 11 साल के अर्ध-आवधिकता के साथ, सूर्य के बड़े पैमाने पर द्विध्रुवीय (उत्तर-दक्षिण) चुंबकीय क्षेत्र घटक भी हर 11 साल में फ़्लिप करता है, हालांकि, द्विध्रुवीय क्षेत्र का शिखर सूर्यस्पॉट संख्या में शिखर को पीछे छोड़ देता है, पूर्व में दो चक्रों के बीच न्यूनतम होता है।

एवररोस ने सनस्पॉट्स को भी समझाया और चंद्रमा के अपारदर्शी रंगों के बारे में एक वैज्ञानिक तर्क दिया, जिसमें उन्होंने तर्क दिया कि चंद्रमा में कुछ हिस्से हैं जो दूसरों की तुलना में मोटे हैं, मोटे हिस्सों को पतले हिस्सों की तुलना में सूर्य से अधिक प्रकाश प्राप्त होता है।

सनस्पॉट इसके अंग्रेजी अर्थ का उदाहरण

Stephanides' professional interest in astronomy dates back to as early as the summer of 1914, when he observed the Sun for two months and made 24 drawings of various groups of sunspots.

Due to Sporadic"nbsp;E propagation during the late spring and most of the summer, regardless of sunspot numbers, afternoon short band openings into small geographic areas of up to 1500"nbsp;km occur.

F2 and TE band openings from other ionospheric reflection/refraction modes, or sky-wave propagation as it is known can also occasionally occur on the low band VHF frequencies of 6 or 4"nbsp;meters, and very rarely on 2"nbsp;meters (high band VHF) during extreme peaks in the 11"nbsp;year sunspot cycle.

Around 4,500 years ago, the capstone upon the summit of the Great Pyramid of Giza absorbed the energy released by the Tartarus Rotation (a monstrous sunspot that occurs every 4,000–4,500 years), and saved the earth from major flooding and catastrophic weather.

In 2006, seven days before this sunspot is again due, the pieces are still divided, and three teams are trying to reunite them: Two for their own gain; one from Europe (representing the Catholic Church); and the other is CIEF, the Commander-in-Chief's In Extremis Force (an American force covertly representing the power of the Freemasons).

There is a rather large sunspot on the Sun's face.

Annie Scott Dill Maunder was a pioneer in astronomical photography, especially of sunspots.

They worked together to observe sunspots and to refine the techniques of solar photography.

Annie's mathematical skills made it possible to analyse the years of sunspot data that Maunder had been collecting at Greenwich.

By analysing the Cambridge records for both sunspots and geomagnetic storm, they were able to show that specific regions of the sun's surface were the source of geomagnetic storms and that the sun did not radiate its energy uniformly into space, as William Thomson, 1st Baron Kelvin had declared.

Numerous astronomical, sunspot, and aurora pictures taken by past and present members.

In early 1946 he turned his attention to sunspots as a source of strong fluctuating radio noise.

The observations confirmed beyond doubt that sunspots were the source of the strong increase in radio noise.