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NEW QUESTION: 1
A. Windows 7
B. Windows 10
C. Windows 8.1
D. Windows 8
Answer: A
NEW QUESTION: 2
Sie haben ein Azure-Abonnement mit dem Namen Abonnement1, das die Ressourcen in der folgenden Tabelle enthält.
VM1 und VM2 führen die Websites in der folgenden Tabelle aus.
AppGW1 verfügt über die Backend-Pools in der folgenden Tabelle.
DNS löst site1.contoso.com, site2.contoso.com und site3.contoso.com in die IP-Adresse von AppGW1 auf.
AppGW1 hat die Listener in der folgenden Tabelle.
AppGW1 hat die Regeln in der folgenden Tabelle.
Wählen Sie für jede der folgenden Anweisungen Ja aus, wenn die Anweisung wahr ist. Andernfalls wählen Sie Nein.
HINWEIS: Jede richtige Auswahl ist einen Punkt wert.
Answer:
Explanation:
Explanation
Vm1 is in Pool1. Rule2 applies to Pool1, Listener 2, and site2.contoso.com
NEW QUESTION: 3
The discoveries of the white dwarf, the neutron star, and the black hole, coming well after the discovery of the red giant are among eh most exciting developments in decades because they may be well present physicists with their greatest challenge since the failure of classical mechanics. In the life cycle of the star, after all of the hydrogen and helium fuel has been burned, the delicate balance between the outer nuclear radiations. Pressure and the stable gravitational force becomes disturbed and slow contraction begins. As compression increases, a very dense plasma forms. If the initial star had mass of less than 1.4 solar masses (1.4 times the mass of our sun), the process ceases at the density of 1,000 tons per cubic inch, and the star becomes the white dwarf. However, if the star was originally more massive, the white dwarf plasma can't resist the gravitations pressures, and in rapid collapse, all nuclei of the star are converted to a gas of free neutrons. Gravitational attraction compresses this neutron gas rapidly until a density of 10 tons per cubic inch is reached; at this point the strong nuclear force resists further contraction. If the mass of the star was between 1.4 and a few solar masses, the process stops here, and we have a neutron star. But if the original star was more massive than a few solar masses, even the strong nuclear forces cannot resist the gravitational brunch. The neutrons are forced into one another to form heavier hadrons and these in turn coalesce to form heavier entities, of which we as yet know nothing. At this point, a complete collapse of the stellar mass occurs; existing theories predict a collapse to infinite density and infinitely small dimensions Well before this, however, the surface gravitational force would become so strong that no signal could ever leave the star - any photon emitted would fall back under gravitational attraction - and the star would become black hole in space. This gravitational collapse poses a fundamental challenge to physics. When the most widely accepted theories predict such improbable things as infinite density and infinitely small dimensions, it simply means that we are missing some vital insight. This last happened in physics in the 1930's, when we faced the fundamental paradox concerning atomic structure. At that time, it was recognized that electrons moved in table orbits about nuclei in atoms. However, it was also recognized that if charge is accelerated, as it must be to remain in orbit, it radiates energy; so, theoretically, the electron would be expected eventually to spiral into the nucleus and destroy the atom.
Studies centered around this paradox led to the development of quantum mechanics. It may well be that an equivalent t advance awaits us in investigating the theoretical problems presented by the phenomenon of gravitational collapse.
According to the passage, an imbalance arises between nuclear radiation pressure and gravitational force in stars because
A. radiation pressure decreases when a star's fuel has been consumed.
B. the collapse of a star increases its gravitational force.
C. radiation pressure increases as a star increases in mass.
D. a dense plasma decreases the star's gravitational force.
E. the density of a star increases as it ages.
Answer: A
Explanation:
Explanation/Reference:
Explanation:
NEW QUESTION: 4
サービスの中断による悪影響を減らすことで、顧客とユーザーの満足度を向上させる方法はどれですか。
A. 変更管理
B. インシデント管理
C. サービスリクエスト管理
D. サービスレベル管理
Answer: B
Explanation:
Explanation
The purpose of incident management is to minimize the negative impact of incidents by restoring normal service operation as quickly as possible. Incident management can have an enormous impact on customer and user satisfaction, and the perception of those stakeholders of the service provider.
https://www.bmc.com/blogs/itil-incident-management/
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