Deployed 0cbd9a7 with MkDocs version: 1.6.0

credits/index.html

@@ -1021,15 +1021,6 @@
     </span>
   </a>
   
-</li>
-      
-        <li class="md-nav__item">
-  <a href="#donators" class="md-nav__link">
-    <span class="md-ellipsis">
-      Donators
-    </span>
-  </a>
-  
 </li>
       
     </ul>
@@ -1082,15 +1073,6 @@
     </span>
   </a>
   
-</li>
-      
-        <li class="md-nav__item">
-  <a href="#donators" class="md-nav__link">
-    <span class="md-ellipsis">
-      Donators
-    </span>
-  </a>
-  
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     </ul>
@@ -1125,68 +1107,6 @@
 <li><a href="https://github.com/ppravatto" title="GitHub profile"><strong>Pierpaolo Pravatto</strong></a> - <em>Wiki page, β Tester</em></li>
 <li><a href="https://github.com/fcapostagno" title="GitHub profile"><strong>Francesco Capostagno</strong></a>, <strong>Luca</strong>, <strong>Pietro</strong> - <em>β Tester</em></li>
 </ul>
-<h2 id="donators">Donators</h2>
-<ul>
-<li>Eric Hahn</li>
-<li>Alan Lawrence</li>
-<li>Diego Gil Fernandez</li>
-<li>Torsten Teichert</li>
-<li>Charles Preston</li>
-<li>Brad Hein</li>
-<li>Paolo Romani</li>
-<li>Michelle Corbani</li>
-<li>Martin van Duinen</li>
-<li>Valentino Zardi</li>
-<li>Emmanuel Fabre</li>
-<li>Oscar Nilsson</li>
-<li>Pierre Declercq</li>
-<li>Detlef Jahn</li>
-<li>Oliver Schellenberg</li>
-<li>Stephane Imbertone</li>
-<li>Roel Ketelaars</li>
-<li>Timothy Ehrhart</li>
-<li>George Mager</li>
-<li>Gerhard Amon</li>
-<li>Gerald Schmidt</li>
-<li>Carlos Rocha</li>
-<li>Joshua Frohberg</li>
-<li>Bill Riches</li>
-<li>Jeffrey Krehbiel</li>
-<li>Володимир Багмет</li>
-<li>Philip Hamlin</li>
-<li>David Davies</li>
-<li>Nigel P. Lawrence</li>
-<li>Marco Rissi (PP5ZX)</li>
-<li>Martin van Duinen</li>
-<li>Alex Diamantopulo</li>
-<li>Joseph Winter</li>
-<li>Mark Bender</li>
-<li>Rolf Gerhardt</li>
-<li>Denese Harris</li>
-<li>Benjamin Steele</li>
-<li>Alexander Irmscher</li>
-<li>Jonathan Chang</li>
-<li>Torsten Lipke</li>
-<li>Massimo Petrantoni</li>
-<li>William Arcand</li>
-<li>Jon Carp</li>
-<li>Robert Crone</li>
-<li>William Houston</li>
-<li>Richard Quasne</li>
-<li>Tom Krugliakov</li>
-<li>Francisco Neira Basso</li>
-<li>Alistair Macrae</li>
-<li>Kevin Arburn</li>
-<li>Marek Barłóg</li>
-<li>Gabriel Glösmann</li>
-<li>Corbin Williams</li>
-<li>Ton Machielsen</li>
-<li>Ivan Rancic</li>
-<li>Alipio Fernandez</li>
-<li>Matt Eisele</li>
-<li>Martin Dudel</li>
-<li>Harald Geier</li>
-</ul>
 
 
 

index.html

@@ -1025,6 +1025,9 @@
     <img alt="Logo" src="assets/logo_large_white.svg#only-dark" width="400" />
 </p>
 <p><strong>Artemis</strong> is a software designed to assist <strong>radio frequency (RF) signal identification and storage</strong>. It simplifies real-time spectrum analysis by leveraging one of the most extensive and community-driven databases, containing nearly <strong>500 recognized signals</strong>. This comprehensive software solution allows users to collect RF signals with specific parameters such as frequency, bandwidth, modulation, etc. Users can also store spectrum waterfalls, audio samples, and all types of documents for future reference. Artemis provides a robust platform to manage a wide range of RF data with precision and ease.</p>
+<p align="center">
+    <a class="md-button" href="https://www.aresvalley.com">Artemis Homepage</a>
+</p>
 
 
 

space_weather/current/index.html

@@ -825,9 +825,9 @@
 </li>
       
         <li class="md-nav__item">
-  <a href="#2-a-index" class="md-nav__link">
+  <a href="#2-ap-index" class="md-nav__link">
     <span class="md-ellipsis">
-      2. A Index
+      2. Ap Index
     </span>
   </a>
   
@@ -1200,9 +1200,9 @@
 </li>
       
         <li class="md-nav__item">
-  <a href="#2-a-index" class="md-nav__link">
+  <a href="#2-ap-index" class="md-nav__link">
     <span class="md-ellipsis">
-      2. A Index
+      2. Ap Index
     </span>
   </a>
   
@@ -1442,8 +1442,8 @@
 </tr>
 </tbody>
 </table>
-<h2 id="2-a-index">2. A Index</h2>
+<h2 id="2-ap-index">2. Ap Index</h2>
-<p>The <strong>A index</strong> represents the three-hourly equivalent amplitude of geomagnetic activity at a specific magnetometer station, derived from the station-specific K index. Due to the quasi-logarithmic nature of the K-scale in relation to magnetometer fluctuations, directly averaging a set of K indices is not really meaningful. Instead each K is converted back into a linear scale. The <strong>Ap index</strong> is determined by averaging the eight daily A values, providing a measure of geomagnetic activity for a specific day. Days with higher levels of geomagnetic activity correspond to higher daily Ap values.</p>
+<p>The <strong>A index</strong> represents the three-hourly equivalent amplitude of geomagnetic activity at a specific magnetometer station, derived from the station-specific K index. Due to the quasi-logarithmic nature of the K-scale in relation to magnetometer fluctuations, directly averaging a set of K indices is not really meaningful. Instead each K is converted back into a linear scale. The <strong>Ap index</strong> is determined by averaging the eight daily Ap values (3-hour) and using the same stations grid explained for the Kp index in the previous section. This provides a measure of geomagnetic activity for a specific day. Days with higher levels of geomagnetic activity correspond to higher daily Ap values.</p>
 <h2 id="3-noaa-space-weather-scale">3. NOAA Space Weather Scale</h2>
 <h3 id="geomagnetic-storm">Geomagnetic Storm</h3>
 <details class="danger">