82. Al-Infitar/Tearing Apart
I/We start by the Blessed Name of Allah
The Immensely Merciful to all, The Infinitely Compassionate to everyone.
82:01
a. The time when the celestial realm will tear apart,
82:02
a. and when the stars/planets will scatter and begin to fall off,
82:03
a. and when the seas/oceans will be made to burst by massive earthquakes and cause a series
of tsunami floods,
82:04
a. and when the graves will be overturned with their burdens of lifeless human bodies,
82:05
a. then every person will know what it did of the good and evil and had sent forward and what it had left behind.
82:06
a. O The People!
b. What is it that lured you away to disbelief from your Gracious Rabb - The Lord in spite of HIS Graciousness and Generosity?
82:07
a. HE is the One WHO created you out of nothingness and without a precedence,
b. then shaped you and proportioned you,
82:08
a. and shaped you in whatever form HE pleased,
b. and configured your composition accordingly.
82:09
a. But no!
b. Even then you deny and belie the reality of the Time of Final Judgment.
82:10
a. You do so while there are ever-watchful angels over you, recording your deeds, speech and dealings,
Surah 82 * Al-Infitar 719
82:11
a. - noble, honorable recorders,
82:12
a. aware of exactly whatever you do and whatever you did.
82:13
a. And, indeed, the righteous will be in bliss of Paradise,
82:14
This study aimed at finding out Islamic education values embedded in the tradition of Merti Deso in Suku Menanti Village, Sindang Jati District, Rejang Lebong Regency, Bengkulu. This study used a descriptive qualitative approach. The data collection techniques used in this study encompassed observation and interviews conducted periodically. After the data were collected, the data were further analyzed by means of Miles, Haberman, and Saldana’s version of stages, namely data selection, data presentation, and drawing conclusion. This study concluded that the Islamic education values embedded in the tradition of Merti Deso were religious and spiritual values, muamalah/social values, and economic values.
A wide range of phenomena related to solar physics, astrophysics and laboratory plasmas contain many features of magnetohydrodynamics (MHD). This thesis presents the numerical studies of classical and relativistic MHD models. In classical MHD, the two dimensional ideal MHD and the shallow water MHD equations are numerically investigated. The third model is a one-dimensional special relativistic MHD (SRMHD) system. These MHD systems are formed by coupling the Maxwell''s equations with the hydrodynamics equations. The simulation of relativistic MHD flows is more difficult due to flow near the speed of light and because of nonlinear relations between conserved and primitive variables. The proposed numerical methods include the space-time conservation element and solution element (CE/SE) method and the kinetic flux vector splitting (KFVS) scheme. In CE/SE solver, the conservation elements are used for calculating the flow variables only, while a central differencing procedure is used to approximate the derivatives of flow variables. The KFVS scheme is based on the direct splitting of macroscopic flux functions of the system. The MUSCL-type reconstruction technique is used to achieve the second order accuracy of the KFVS method. For the designed MHD codes, the projection method is used to satisfy the divergence-free constraint associated with the magnetic field. For validation and comparison, the central scheme is applied to the investigated models. The case studies of ideal MHD include the MHD Kelvin- Helmholtz instability, the MHD rotor problem, the MHD shock interaction with clouds, the blast wave problem and the very famous Orszag-Tang MHD turbulence problem. In the SRMHD case, the one-dimensional relativistic Riemann problems, the interaction of shock fronts, and the relativistic blast wave problems are studied. In all test cases, the suggested computational techniques produced accurate results efficiently.