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Enregistrement W2617749117 · doi:10.2505/4/tst17_084_03_33

Total Eclipse: The Solar Eclipse this August is An Ideal Opportunity to Practice Three-Dimensional Science Learning

2017· article· en· W2617749117 sur OpenAlexaboutno aff
Dennis Schatz, A. Fraknoi

Notice bibliographique

RevueThe Science Teacher · 2017
Typearticle
Langueen
DomaineBusiness, Management and Accounting
ThématiqueAttention Economy in Education and Business
Établissements canadiensnon disponible
Organismes subventionnairesnon disponible
Mots-clésSolar eclipseBeautyEclipseAtmosphere (unit)SociologyMeteorologyPhysicsAstronomyLawPolitical science

Résumé

récupéré en direct d'OpenAlex

[ILLUSTRATION OMITTED] [FIGURE 1 OMITTED] This summer, on August 21, 500 million people across North America will experience one of the most beautiful astronomical phenomena: an eclipse of the Sun. It will be a must teach moment, when all students will want to know the what, when, and of the event. In addition, many high school science teachers are likely to be asked about it, not only in their classes, but in discussions with colleagues, family, and community members. Research shows that many high school students--and adults--fail to correctly understand the Earth-Sun-Moon system (Hermann and Lewis 2003). If you are lucky enough to be in the 100-kilometer-wide path of totality, you will see the Moon completely cover the Sun. When only a sliver of sunlight is visible, your surroundings will darken, as if the Sun were setting. Temperatures will drop, and birds will go to roost, thinking that night is coming. Finally, the Sun will be totally covered, and the beautiful solar atmosphere (the corona) will become visible (Figure 1). Totality will last about two minutes for this eclipse, depending on location, and then the Sun will slowly be uncovered. While only those people in the narrow 100-kilometerwide band will see a total eclipse, everyone in the United States (as well as Canada and Mexico) will see at least a partial eclipse (Figure 1), where a big bite is taken out of the Sun. Teachers, students, and families will want to enjoy its beauty and will need to be prepared to safely observe the event. More information regarding where and when the eclipse is visible, plus safe viewing strategies, are in the insert in this issue of The Science Teacher. The insert can also be accessed online (see On the web). By August, we expect enormous media and public interest in the eclipse and how to observe and understand it. Science teachers can help students and communities prepare. Eclipses are rare and exciting events that generally produce a feeling of cosmic awe and mystery, but people's sense of wonder can be further enhanced by a clear understanding of what causes them. Indeed, the 2017 eclipse provides a great hook to engage students in wanting to know what causes the phases of the Moon (key to understanding eclipses), how and when we get solar and lunar eclipses, and why people travel thousands of miles and spend thousands of dollars to see a total solar eclipse. The eclipse and three-dimensional science learning For educators, the eclipse and its associated ideas provide the perfect opportunity to incorporate three-dimensional learning (3-D learning) into your teaching, as recommended by the Next Generation Science Standards (NGSS Lead States 2013; see box, p. 38), covering science and engineering practices (SEPs), disciplinary core ideas (DCIs), and crosscutting concepts (CCs). The goal of 3-D learning is to interweave the dimensions, so students see them as a connected whole. Not every individual activity lends itself to incorporating all three dimensions. It is only when you look at a sequence of learning experiences that one can identify effective ways to incorporate 3-D learning. Helping students to understand what causes solar eclipses provides an ideal opportunity to connect a number of learning experiences over several weeks. These not only incorporate 3-D learning but also include other essential learning strategies, such as assessing prior student understanding of the subject and assessing the learning that occurs during and after instruction. 3-D learning in action So, how does 3-D learning actually work in the classroom? The following set of learning experiences asks students to demonstrate their current understanding of lunar phases before they learn what causes these phases and then finally gain a full understanding of solar and lunar eclipses. These activities come from our book, Solar Science: Exploring Sunspots, Seasons, Eclipses and More, available from NSTA Press (Schatz and Fraknoi 2016). …

Récupéré en direct depuis OpenAlex et désinversé. Les résumés ne sont pas conservés dans cette base de données : les index inversés représentent 8,6 Go des 9,3 Go de texte de la base, et le serveur dispose de 13 Go libres.

Comment cette classification a été obtenuedéplier

Prédiction machine sur la base complète

Imitation des enseignants

Ni prévalence calibrée, ni vérité terrain. Validation humaine à venir. Le volet Gemma est une étiquette directe du modèle pour chaque travail de la base, lue sur la notice réduite au titre. Le volet Codex est un classifieur appris des 10 348 étiquettes directes de Codex et calibré sur les taux pondérés de l'échantillon; les champs sans appui suffisant ne portent aucun appel Codex. Le mode candidate est l'union des deux volets; le consensus est leur intersection. Ces sorties portent le statut machine_predicted_unvalidated et ne sont pas des étiquettes humaines.

score de la tête « metaresearch » (Codex)0,001
score de la tête « metaresearch » (Gemma)0,002
Version: metacan-v3-hybrid-931329e0061cStatut de validation: machine_predicted_unvalidated
Catégories candidatesaucune
Catégories consensuellesaucune
DomaineSignal candidat: aucune · Signal consensuel: aucune
Devis d'étudeSignal candidat: Sans objet · Signal consensuel: Sans objet
GenreSignal candidat: Autre · Signal consensuel: Autre
Score de désaccord entre enseignants0,153
Score d'incertitude au seuil0,512

Scores du classifieur distillé par catégorie (deux têtes)

CatégorieCodexGemma
Métarecherche0,0010,002
Méta-épidémiologie (sens strict)0,0010,000
Méta-épidémiologie (sens large)0,0000,001
Bibliométrie0,0000,000
Études des sciences et des technologies0,0020,001
Communication savante0,0030,003
Science ouverte0,0010,005
Intégrité de la recherche0,0020,002
Charge utile insuffisante (le modèle a refusé de juger)0,1530,064

Scores machine (provisoires)

Les deux têtes enseignantes du modèle étudiant, lues sur ce travail. Un score ordonne la base pour la relecture; il n'affirme jamais une catégorie, et le statut de validation accompagne chaque rangée tel quel.

Scores de référence d'un modèle non mature (critères de maturité non atteints, 7 itérations). Un score ordonne; il n'affirme jamais une catégorie.

Tête enseignante Opus0,073
Tête enseignante GPT0,334
Écart entre enseignants0,262 · la distance entre les deux têtes enseignantes sur ce seul travail
Statut de validationscore_only:v0-immature-baseline · tel quel depuis la passe de notation : score_only signifie que le nombre peut ordonner les travaux, et qu'aucune étiquette de catégorie n'en découle

Classification

machine, non validée

Prédiction automatique; un appel candidat d’une seule source (Gemma direct ou Codex distillé), pas un consensus.

Les modèles n’ont appliqué aucune catégorie : rien dans la taxonomie ne correspondait à ce travail.
Devis d'étudeSans objet
Domainenon disponible
GenreAutre

Le détail, modèle par modèle et score par score, se trouve en fin de page sous « Comment cette classification a été obtenue ».

En bref

Citations0
Publié2017
Routes d'admission1
Résumé présentoui

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