Whitney Houston's Funeral Shows Trouble Already Brewing Around Her Estate

Whitney Houston’s funeral this weekend provided the first public glimpse of what may be trouble involving her estate. Her ex-husband, Bobby Brown, was invited to the funeral, after reports surfaced that some family members didn’t want him there. He didn’t last long. Brown’s entourage wasn’t allowed to sit with him at the funeral. Brown wasn’t happy and left, visibly upset.


Bobby Brown issued a statement after the funeral, saying he and his group were asked to relocate three times, and rather than making a scene, he chose to pay his respects quickly and leave.

TMZ reported the day before the funeral that Whitney’s mother, Cissy Houston, and other family members had been trying to keep Brown away from Bobbi Kristina, Whitney’s daughter with Brown. They were said to be worried that Brown would try to use Bobbi Kristina to make a play for some of Whitney’s money.

Brown’s statement confirmed some of this. He said that security prevented him from seeing his daughter at the funeral. Is money the reason why? Brown tried to get some of Whitney’s money through a court proceeding in 2007, just after their divorce judgment was entered, but he failed.

Some have speculated that Whitney’s estate will be worth between $1

Solar Flares

A solar flare is a sudden brightening observed over the Sun surface or the solar limb, which is interpreted as a large energy release of up to 6 × 1025 joules of energy[1] (about a sixth of the total energy output of the Sun each second) or 160,000,000,000 megatons of TNT equivalent, over 25,000 times more energy released from the impact of Comet_Shoemaker–Levy_9 with Jupiter. The flare ejects clouds of electrons, ions, and atoms through the corona into space. These clouds typically reach Earth a day or two after the event.[2] The term is also used to refer to similar phenomena in other stars, where the term stellar flare applies.

Solar flares affect all layers of the solar atmosphere (photosphere, chromosphere, and corona), when the medium plasma is heated to tens of millions of kelvins and electrons, protons, and heavier ions are accelerated to near thespeed of light. They produce radiation across the electromagnetic spectrum at all wavelengths, from radio waves to gamma rays, although most of the energy goes to frequencies outside the visual range and for this reason the majority of the flares are not visible to the naked eye and must be observed with special instruments. Flares occur in active regions around sunspots, where intense magnetic fields penetrate the photosphere to link the corona to the solar interior. Flares are powered by the sudden (timescales of minutes to tens of minutes) release of magnetic energy stored in the corona. The same energy releases may produce coronal mass ejections (CME), although the relation between CMEs and flares is still not well established.

Solar Flares

X-rays and UV radiation emitted by solar flares can affect Earth's ionosphere and disrupt long-range radio communications. Direct radio emission at decimetric wavelengths may disturb operation of radars and other devices operating at these frequencies.

Solar flares were first observed on the Sun by Richard Christopher Carrington and independently by Richard Hodgson in 1859 [3] as localized visible brightenings of small areas within a sunspot group. Stellar flares have also been observed on a variety of other stars.

The frequency of occurrence of solar flares varies, from several per day when the Sun is particularly "active" to less than one every week when the Sun is "quiet", following the 11-year cycle (the solar cycle). Large flares are less frequent than smaller ones.

Blogger Şablon Genişletme

Blogumuza temamızı yükledik fakat baktık ki içerik ya da reklam alanı koymak için yeterince yer yok.Peki ne yapacağız? Üzerinde uğraştığımız temamızı bir anda silecek miyiz yoksa temamızı genişletmeyi mi deneyeceğiz? Seçim size kalmış ama şablon genişletme yaparak istediğiniz sonuca %90 ulaşabilirsiniz.Nasıl mı?

İlk olarak Yerleşim / HTML'yi Düzenle'ye giriyoruz ve Widget Şablonlarını Genişlet'e tıklıyoruz.

İlk olarak örnek verelim.Diyelim ki değerlerimiz :

#outer-wrapper {
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width: 1000px;


#main-wrapper {
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width: 700px;


#sidebar-wrapper {
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width: 300px;



.post-body pre {
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width: 670px;

olsun ve biz şablonumuzu genişletmek istiyoruz.Mantık kolay aslında.Bir taraf ne kadar artarsa diğer taraf da o kadar artacak.Buna göre şablon genişliğimiz 1000px ise biz bunu nasıl 1400px çevirebiliriz? İşte böyle :

#outer-wrapper {
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width: 1400px;


#main-wrapper {
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width: 1000px;


#sidebar-wrapper {
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width: 400px;



.post-body pre {
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width: 970px;

Aslında ben bunu öylesine yaptım.isterseniz 1400pxi 900-500 , 800-600, 1100-300, 1200-200 olarak ayarlayabilirsiniz.