en:vlf_data
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====== VLF Data Analysis ====== | ====== VLF Data Analysis ====== | ||
**What do we measure by the SID monitors?** \\ | **What do we measure by the SID monitors?** \\ | ||
- | The SID monitors are inductive | + | |
+ | The SID monitors are inductive | ||
The plot describing how the measured data look like is shown.\\ | The plot describing how the measured data look like is shown.\\ | ||
[[https:// | [[https:// | ||
- | SID measurement from March 6, 2016. A strong fireball was detected that day. In this plot, we can see some peaks corresponding with the fireballs’ | + | {{: |
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Basicly, we use polynomial differential equations to describe the electron plasma frequency. We know the middle value which also equals 23.4 kHz. It means that the photon spreading through the plasma is refracted by the electrons with the same oscillation frequency. However, the electron plasma frequency changes and it’s numerical solution is the result of our basic equation, indeed. The grap his given if Figure 2.\\ | Basicly, we use polynomial differential equations to describe the electron plasma frequency. We know the middle value which also equals 23.4 kHz. It means that the photon spreading through the plasma is refracted by the electrons with the same oscillation frequency. However, the electron plasma frequency changes and it’s numerical solution is the result of our basic equation, indeed. The grap his given if Figure 2.\\ | ||
- | [[https:// | + | [[https:// |
- | Electron plasma frequency of the ionospheric plasma measured on March 6, 2016. | + | {{: |
+ | \\ | ||
We can deduce that the electrons oscillate among heavy ions with variable amplitude and frequency, which is important to determine the current electron density, too.\\ | We can deduce that the electrons oscillate among heavy ions with variable amplitude and frequency, which is important to determine the current electron density, too.\\ | ||
If the electron plasma frequency is known, we can compute the ionospheric electron density. Actually, it’s known that the electron’s oscillation frequency is the total function of the amount of electrons and heavy ions. Applying the appropriate equation we get the momental electron density shown in Figure 3. \\ | If the electron plasma frequency is known, we can compute the ionospheric electron density. Actually, it’s known that the electron’s oscillation frequency is the total function of the amount of electrons and heavy ions. Applying the appropriate equation we get the momental electron density shown in Figure 3. \\ | ||
[[https:// | [[https:// | ||
- | The ionospheric electron density modeled using the electron plasma frequence. \\ | + | {{: |
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Within the system of differential equaitons with electron density included, we can also approach the height where an impact reached the ionosphere. These plots where electron density is compared with height are called ionograms. The ionogram from March 6, 2016 is given. Height is approximated as the function of electron density’s derivation and the whole phenomenon is compared in time, too. Some stronger impacts can be seen and recognized easily. \\ | Within the system of differential equaitons with electron density included, we can also approach the height where an impact reached the ionosphere. These plots where electron density is compared with height are called ionograms. The ionogram from March 6, 2016 is given. Height is approximated as the function of electron density’s derivation and the whole phenomenon is compared in time, too. Some stronger impacts can be seen and recognized easily. \\ | ||
[[https:// | [[https:// | ||
- | The ionospheric plasma ionogram from March 6, 2016. | + | {{: |
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We are able to work out how the impacts affected ionization and recombination in the low - temperature ionospheric plasma. By the time these parameters are known, we can use a system of other differential equations to compute the electron density and temperature of the fireball and plasma located to surround the solid. We can even form the contour plot of the temperature-dependent electron density’s distribution and approach the chemical emission spectra of the investigated fireball. We deduced that the shiny fireball detected on March 6, 2016 might have been consisted of some pyroxenes. The electron density, temperature and their distribution models are given. \\ | We are able to work out how the impacts affected ionization and recombination in the low - temperature ionospheric plasma. By the time these parameters are known, we can use a system of other differential equations to compute the electron density and temperature of the fireball and plasma located to surround the solid. We can even form the contour plot of the temperature-dependent electron density’s distribution and approach the chemical emission spectra of the investigated fireball. We deduced that the shiny fireball detected on March 6, 2016 might have been consisted of some pyroxenes. The electron density, temperature and their distribution models are given. \\ | ||
- | [[https:// | + | [[https:// |
- | Graph describing the fireball’s temperature is shown. \\ | + | {{: |
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[[https:// | [[https:// | ||
- | Fireball’s electron density is shown. \\ | + | {{: |
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[[https:// | [[https:// | ||
- | The temperature - dependent electron density’s distribution was modeled. We can see that another plasma discharge was fired up in the ionized cover surrounding the solid, out of the core. Some alkali metals might have been present in that discharge. \\ | + | {{: |
+ | \\ | ||
en/vlf_data.1460064451.txt.gz · Last modified: 2016/04/07 21:27 (external edit)