Ehille crescent visibility
Author: J | 2025-04-24
stable EHILLE Crescent Visibility () ios torrentdownloads microsoft gratuite version EHILLE Crescent Visibility RapidShare german torrent tpb comment installer
EHILLE Crescent Visibility - software-repository.com
The resulting visibility algorithm is sketched below. − Time, date, time zone − Latitude, longitude − Altitude, probability (P) The algorithm claimed can be sketched as a graph, displaying S max (y-axis) vs. M (x-axis) for various crescent widths (W) in Figure 9: Calculate: − Sun Altitude (S) − Moon Altitude (M) − Crescent Width (W) − Sight Elevation (E) M > -0.5 – E NO YES Figure 9 – Visibility Graph of Proposed Criterion NO M 4 M = 4 YES YES X = 10 * M – 56 To demonstrate the performance of the criterion and compare its results with the other criteria in literature, a tiny software program 2 has been developed as a screen saver. EHILLE, this screen saver, can be easily configured to supply the necessary parameters (Figure 10). X = M – 20 S max = (X + 10 * W) / 3 S’ max = S max + E S’’ max = S’ max – P / 50 + 1 YES S’’ max > 4 OR S The area of instantaneous visibility is painted on a Mercator map in real-time and the painted areas are then combined to form the cumulative area of visibility, which has the shape of a parabola. The vertex of this parabola represents the “best place” on Earth and the area widens westward, being symmetric on a roughly horizontal line. The position of the vertex is unique for each lunation. The software first computes the time of conjunction and shifts the Mercator map accordingly, such that the parabola lies more or less on the same place, its vertex being placed near the right border. Next is calculated the start time, which is nearly one hour before the first global visibility. Then the time is progressed with the entered speed and the visibility is checked continually. A relatively simple approach to draw the parabola would be to compute the visibility for each pixel (corresponding to a certain latitude & longitude) by executing the novel algorithm for every tested time. However, this necessitates more than 500 million loops for a complete. stable EHILLE Crescent Visibility () ios torrentdownloads microsoft gratuite version EHILLE Crescent Visibility RapidShare german torrent tpb comment installer EHILLE Crescent Visibility Crack X64 [2025] Download EHILLE Crescent Visibility Free Download [Mac/Win] (Latest) EHILLE Crescent Visibility Activation Code is a light-weight application that features an easy-to-use interface. The program will allow you to adjust the algorithm to get different results from the visibility of the moon on the map of different results from the visibility of the moon on the map of the world, depending on the day and time you want to monitor. Visualization of the visibility of the moon on the map of the world. Easy to use interface, with various configuration options. EHILLE Crescent Visibility Screenshots: EHILLE Crescent Visibility Main Interface: EHILLE gratuite version EHILLE Crescent Visibility RapidShare german torrent tpb comment installer stable EHILLE Crescent Visibility turbobit original o peut t l charger gratuite version EHILLE Crescent Visibility RapidShare german torrent tpb comment installer stable EHILLE Crescent Visibility turbobit original o peut t l charger android nacutesuppcor35 Subscribe gratuite version EHILLE Crescent Visibility RapidShare german torrent tpb comment installer stable EHILLE Crescent Visibility turbobit original o peut t l charger android nacutesuppcor35 Subscribe EHILLE Crescent Visibility is a lightweight piece of software designed as a screensaver that is meant to trace the visibility of the moon on Run, requiring a huge amount of calculation time. Therefore the software uses a smart search & track method which speeds up the process nearly 5,000-fold, as detailed below. Following the start, the software searches the best place on the map for visibility. Beginning from the center of the right border, a vertical search (up and down) is performed as to maximize ARCV to find the latitude where the Moon is vertical to the Sun (DAZ = 0). Consecutively, a horizontal search determines the longitude where the Moon altitude is 4°, which is most favorable condition according to our algorithm. The combined search fixes the position with the highest possibility of visibility, and this position is tested & updated only once for each time using the algorithm. The time is then incremented one minute and the search is repeated. After detection of the maiden visibility at this best place, the coordinates & local time is displayed on the screen. Now, the software checks the visibility in a vertical scan and saves the latitude limits of visibility, up and down, which forms the border points of the parabola. The connection line is then painted. This scan is repeated for neighbor longitudes, left and right, until visibility ceases. The instantaneous visibility area is formed thereby. For the next minute, the software shifts the former “best place” to left (¼°) and the horizontal scan is initiated from the saved points, considerably shrinking the computing time. A screenshot of the tool is displayed in Figure 11 to visualize the output. The graph looks very similar to those obtained through the famous Moon Calculator program by Dr. Monzur Ahmed. Figure 11 – Visibility Parabola Obtained by EHILLE 6. COMPARISON & CONCLUSION Several cases will be analyzed in this section and compared with the criteria available in literature, as to evaluate the validity of the proposed method. Since our criteria uses topocentric Moon elevation, we will consider the parallax of Moon (≈ 0.95°) for the calculation of the error. Case #1: DAZ = 0°, ARCV = 10.5° This case is the upper-left corner of the mean ofComments
The resulting visibility algorithm is sketched below. − Time, date, time zone − Latitude, longitude − Altitude, probability (P) The algorithm claimed can be sketched as a graph, displaying S max (y-axis) vs. M (x-axis) for various crescent widths (W) in Figure 9: Calculate: − Sun Altitude (S) − Moon Altitude (M) − Crescent Width (W) − Sight Elevation (E) M > -0.5 – E NO YES Figure 9 – Visibility Graph of Proposed Criterion NO M 4 M = 4 YES YES X = 10 * M – 56 To demonstrate the performance of the criterion and compare its results with the other criteria in literature, a tiny software program 2 has been developed as a screen saver. EHILLE, this screen saver, can be easily configured to supply the necessary parameters (Figure 10). X = M – 20 S max = (X + 10 * W) / 3 S’ max = S max + E S’’ max = S’ max – P / 50 + 1 YES S’’ max > 4 OR S The area of instantaneous visibility is painted on a Mercator map in real-time and the painted areas are then combined to form the cumulative area of visibility, which has the shape of a parabola. The vertex of this parabola represents the “best place” on Earth and the area widens westward, being symmetric on a roughly horizontal line. The position of the vertex is unique for each lunation. The software first computes the time of conjunction and shifts the Mercator map accordingly, such that the parabola lies more or less on the same place, its vertex being placed near the right border. Next is calculated the start time, which is nearly one hour before the first global visibility. Then the time is progressed with the entered speed and the visibility is checked continually. A relatively simple approach to draw the parabola would be to compute the visibility for each pixel (corresponding to a certain latitude & longitude) by executing the novel algorithm for every tested time. However, this necessitates more than 500 million loops for a complete
2025-04-23Run, requiring a huge amount of calculation time. Therefore the software uses a smart search & track method which speeds up the process nearly 5,000-fold, as detailed below. Following the start, the software searches the best place on the map for visibility. Beginning from the center of the right border, a vertical search (up and down) is performed as to maximize ARCV to find the latitude where the Moon is vertical to the Sun (DAZ = 0). Consecutively, a horizontal search determines the longitude where the Moon altitude is 4°, which is most favorable condition according to our algorithm. The combined search fixes the position with the highest possibility of visibility, and this position is tested & updated only once for each time using the algorithm. The time is then incremented one minute and the search is repeated. After detection of the maiden visibility at this best place, the coordinates & local time is displayed on the screen. Now, the software checks the visibility in a vertical scan and saves the latitude limits of visibility, up and down, which forms the border points of the parabola. The connection line is then painted. This scan is repeated for neighbor longitudes, left and right, until visibility ceases. The instantaneous visibility area is formed thereby. For the next minute, the software shifts the former “best place” to left (¼°) and the horizontal scan is initiated from the saved points, considerably shrinking the computing time. A screenshot of the tool is displayed in Figure 11 to visualize the output. The graph looks very similar to those obtained through the famous Moon Calculator program by Dr. Monzur Ahmed. Figure 11 – Visibility Parabola Obtained by EHILLE 6. COMPARISON & CONCLUSION Several cases will be analyzed in this section and compared with the criteria available in literature, as to evaluate the validity of the proposed method. Since our criteria uses topocentric Moon elevation, we will consider the parallax of Moon (≈ 0.95°) for the calculation of the error. Case #1: DAZ = 0°, ARCV = 10.5° This case is the upper-left corner of the mean of
2025-04-03Dubai: The crescent moon of Sha'ban, the eighth month of the Islamic lunar calendar, will form following the conjunction of the sun and moon at 4:46 PM on Wednesday, January 29, 2025, according to Ibrahim Al Jarwan, Chairman of the Emirates Astronomy Society.Al Jarwan noted that observing the crescent moon on the same evening will be impossible, but visibility is expected on Thursday evening, January 30, 2025.Based on astronomical calculations, Friday, January 31, will mark the beginning of Sha'ban, leaving just one month until the start of Ramadan.The exact start of Ramadan, observed by Muslims worldwide, is determined by a moon-sighting committee. The ninth month of the Islamic lunar calendar is marked by fasting from dawn to dusk, increased prayers, and acts of charity, commemorating the Quran’s revelation to the Prophet Muhammad (PBUH).During Ramadan, the UAE enforces shorter work hours under labor laws, reducing the standard eight-hour workday to six hours.
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