Solar energy is an inexhaustible source of energy that can be converted directly or indirectly into heat and electricity. The sun is expected to radiate at a constant rate for billions of years. It has the greatest potential of all renewable energy sources, but its diffuse nature and intermittency present challenges. Solar radiation is measured as the amount of energy received per unit time and area from the top of the atmosphere, known as the solar constant, which NASA estimates is approximately 1353 watts per square meter.
This presentation contains Basic introduction of sun and solar power, Technical terminologies related to solar power, Electromagnetic Spectrum,Sun Earth relationships,Types of Solar Radiation,Principles of measurement of Solar Radiation,
Solar radiation measurement Instruments,
Solar Photo Voltaic System,P-N Junction,Solar Cell,Types of Solar Cells,SOLAR COLLECTORS and recent trades of solar power utilization
Here is the 2nd project of mine, given by college students. get information from this. want to create like this contact me @instagram slide+ presentation
10
الزملاء الأفاضل
نرحب بحضراتكم مع انطلاق
مبادرة #تواصل_تطوير
المحاضرة العاشرة من المبادرة مع
الأستاذ الدكتور/عبدالرحمن الليثي
الأستاذ المشارك بجامعة الملك سعود
بعنوان
"الطاقة الشمسية واتجاهاتها الحديثة"
العاشرة مساء بتوقيت مكة المكرمة الاثنين11مايو2020
وذلك عبر تطبيق زووم وقناة اليوتيوب الخاصة بالجمعية
https://www.linkedin.com/events/6665350460062474242
علما ان هناك بث مباشر للمحاضرة على القنوات الخاصة بجمعية المهندسين المصريين
ونأمل أن نوفق في تقديم ما ينفع المهندس ومهمة الهندسة في عالمنا العربي
والله الموفق
ملاحظة : تجنبا لاي ظروف, لطفا المشاركة على قناة التليجرام للحصول على دعوات المحاضرات على ZOOM
رابط اللينكدان
www.linkedin.com/company/eeaksa-egyptian-engineers-association/
رابط قناة التليجرام
https://t.me/EEAKSA
رابط قناة الفيسبوك
https://www.facebook.com/EEAKSA
رابط قناة اليوتيوب
https://www.youtube.com/user/EEAchannal
رابط التسجيل العام للمحاضرات
https://forms.gle/vVmw7L187tiATRPw9
This presentation contains Basic introduction of sun and solar power, Technical terminologies related to solar power, Electromagnetic Spectrum,Sun Earth relationships,Types of Solar Radiation,Principles of measurement of Solar Radiation,
Solar radiation measurement Instruments,
Solar Photo Voltaic System,P-N Junction,Solar Cell,Types of Solar Cells,SOLAR COLLECTORS and recent trades of solar power utilization
Here is the 2nd project of mine, given by college students. get information from this. want to create like this contact me @instagram slide+ presentation
10
الزملاء الأفاضل
نرحب بحضراتكم مع انطلاق
مبادرة #تواصل_تطوير
المحاضرة العاشرة من المبادرة مع
الأستاذ الدكتور/عبدالرحمن الليثي
الأستاذ المشارك بجامعة الملك سعود
بعنوان
"الطاقة الشمسية واتجاهاتها الحديثة"
العاشرة مساء بتوقيت مكة المكرمة الاثنين11مايو2020
وذلك عبر تطبيق زووم وقناة اليوتيوب الخاصة بالجمعية
https://www.linkedin.com/events/6665350460062474242
علما ان هناك بث مباشر للمحاضرة على القنوات الخاصة بجمعية المهندسين المصريين
ونأمل أن نوفق في تقديم ما ينفع المهندس ومهمة الهندسة في عالمنا العربي
والله الموفق
ملاحظة : تجنبا لاي ظروف, لطفا المشاركة على قناة التليجرام للحصول على دعوات المحاضرات على ZOOM
رابط اللينكدان
www.linkedin.com/company/eeaksa-egyptian-engineers-association/
رابط قناة التليجرام
https://t.me/EEAKSA
رابط قناة الفيسبوك
https://www.facebook.com/EEAKSA
رابط قناة اليوتيوب
https://www.youtube.com/user/EEAchannal
رابط التسجيل العام للمحاضرات
https://forms.gle/vVmw7L187tiATRPw9
Effect of Shading Devices, Infiltartion-stack effect, wind pressures, Internal Heat Gains, System Heat gain, cooling and heating load estimates, Energy conservations in airconditioning buildings
Physical Geography Lecture 04 - Earth's Energy and Seasons 10.03.16angelaorr
Earth In Space. Variations in Earth's Motion. Earth's Orbit. Axial Tilt. Solstices and Equinoxes. Properties of Electromagnetic Radiation. Insolation and the Solar Constant.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
Richard's aventures in two entangled wonderlandsRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
Cancer cell metabolism: special Reference to Lactate PathwayAADYARAJPANDEY1
Normal Cell Metabolism:
Cellular respiration describes the series of steps that cells use to break down sugar and other chemicals to get the energy we need to function.
Energy is stored in the bonds of glucose and when glucose is broken down, much of that energy is released.
Cell utilize energy in the form of ATP.
The first step of respiration is called glycolysis. In a series of steps, glycolysis breaks glucose into two smaller molecules - a chemical called pyruvate. A small amount of ATP is formed during this process.
Most healthy cells continue the breakdown in a second process, called the Kreb's cycle. The Kreb's cycle allows cells to “burn” the pyruvates made in glycolysis to get more ATP.
The last step in the breakdown of glucose is called oxidative phosphorylation (Ox-Phos).
It takes place in specialized cell structures called mitochondria. This process produces a large amount of ATP. Importantly, cells need oxygen to complete oxidative phosphorylation.
If a cell completes only glycolysis, only 2 molecules of ATP are made per glucose. However, if the cell completes the entire respiration process (glycolysis - Kreb's - oxidative phosphorylation), about 36 molecules of ATP are created, giving it much more energy to use.
IN CANCER CELL:
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
introduction to WARBERG PHENOMENA:
WARBURG EFFECT Usually, cancer cells are highly glycolytic (glucose addiction) and take up more glucose than do normal cells from outside.
Otto Heinrich Warburg (; 8 October 1883 – 1 August 1970) In 1931 was awarded the Nobel Prize in Physiology for his "discovery of the nature and mode of action of the respiratory enzyme.
WARNBURG EFFECT : cancer cells under aerobic (well-oxygenated) conditions to metabolize glucose to lactate (aerobic glycolysis) is known as the Warburg effect. Warburg made the observation that tumor slices consume glucose and secrete lactate at a higher rate than normal tissues.
A brief information about the SCOP protein database used in bioinformatics.
The Structural Classification of Proteins (SCOP) database is a comprehensive and authoritative resource for the structural and evolutionary relationships of proteins. It provides a detailed and curated classification of protein structures, grouping them into families, superfamilies, and folds based on their structural and sequence similarities.
2. Solar Radiation and Measurements.
• Solar Energy can be converted either directly or indirectly
into other forms of energy such as heat and electricity.
• The sun is expected to radiate at an essentially constant rate
for a few billion years.
• So inexhautsible source of energy
• Solar energy reaching at the top of the atmosphere
8% UV radiation
46%Visible Light
46% Infrared Radiation
3. Solar Energy
• Major source of power
• Greatest potential of all the renewable sources
• Its potential – 178 billion MW
• About 20000 times the world’s demand
• Solar power where sun hits atmosphere - 1017W
• Solar power on earth’s surface - 1016W
Main Limitations
• Solar light is diffuse not concentrated
• Large space is required.
• Intermittent and variable manner in which it arrives at the
earth’s surface
• Presence of clouds, wind, haze etc.
4. Solar Constant - Isc
• The rate at which solar energy arrives at the top of the
atmosphere
• Solar Constant is the amount of energy received
• In unit time
• On a unit area
• Perpendicular to the sun’s direction
• At the mean distance of the earth from the Sun
• Since Sun’s activities vary, rate of arrival of solar radiation also
varies
• actual value – avg of these values (may vary about 3% on either
direction)
5. Contd……
NASA standard value of solar constant in three different units
• 1.353 kilowatts per square meter or 1353 watt per sq m
• 116.5 langleys (calories per sq. cm) per hour, or 1165 kcal
per sq m per hr (1 langley = 1cal/cm2)
• 429.2 Btu per sq ft per hour. (1 British thermal Unit Btu =
1055 J)
7. Beam Radiation
• Solar radiation that has not been absorbed or scattered and
reaches the ground directly from the Sun is direct or beam
radiation
•It produces a shadow when interrupted by an opaque object
Diffuse Radiation
•Solar radiation received from the Sun after its direction has
been changed by reflection and scattering from the atmosphere.
•Since scattered in all directions diffuse radiation comes from all
parts of the sky
Total or Global Radiation
Sum of direct and diffuse radiation